{"id":55,"date":"2021-08-26T09:28:45","date_gmt":"2021-08-26T00:28:45","guid":{"rendered":"http:\/\/agarc.sci.kagoshima-u.ac.jp\/wordpress\/?page_id=55"},"modified":"2026-03-18T11:47:06","modified_gmt":"2026-03-18T02:47:06","slug":"danwakai","status":"publish","type":"page","link":"https:\/\/agarc.sci.kagoshima-u.ac.jp\/ja\/danwakai\/","title":{"rendered":"\u9e7f\u5150\u5cf6\u5927\u5b66\u5929\u6587\u5b66\u8ac7\u8a71\u4f1a"},"content":{"rendered":"
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\u7814\u7a76\u8005\u306e\u65b9\u3078\u304a\u77e5\u3089\u305b<\/a><\/div>\n
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\u9e7f\u5150\u5cf6\u5927\u5b66\u7406\u5b66\u90e8\u5929\u6587\u5b66\u8ac7\u8a71\u4f1a\u3068\u306f\u3001\u5b87\u5b99\u7269\u7406\u5b66\u7814\u7a76\u5ba4\u306e\u5b66\u751f\u3084\u30b9\u30bf\u30c3\u30d5\u3092\u4e3b\u305f\u308b\u5bfe\u8c61\u3068\u3057\u3066\u3001\u9e7f\u5150\u5cf6\u5927\u5b66\u3092\u8a2a\u308c\u3066\u3044\u308b\u5929\u6587\u5b66\u7814\u7a76\u8005\u304c\u81ea\u3089\u306e\u7814\u7a76\u6210\u679c\u3092\u4e2d\u5fc3\u306b\u7d39\u4ecb\u3059\u308b\u4f1a\u5408\u3067\u3059\u3002\u4e0d\u5b9a\u671f\u306b\u958b\u50ac\u3055\u308c\u307e\u3059\u306e\u3067\u3001\u8208\u5473\u304c\u3042\u308b\u65b9\u306f\u7a4d\u6975\u7684\u306b\u53c2\u52a0\u3057\u3066\u4e0b\u3055\u3044\u3002\uff08\u5b87\u5b99\u7269\u7406\u5b66\u7814\u7a76\u5ba4\u306b\u6240\u5c5e\u3057\u3066\u3044\u306a\u3044\u4eba\u3067\u3082\u8074\u8b1b\u53c2\u52a0\u3067\u304d\u307e\u3059\uff09\u8b1b\u5e2b\u306b\u306f\u539f\u5247\u3068\u3057\u3066\u65c5\u8cbb\u63f4\u52a9\u3084\u8b1d\u91d1\u306f\u652f\u7d66\u3055\u308c\u307e\u305b\u3093\u3002\u8a00\u8a9e\u306f\u65e5\u672c\u8a9e\u304c\u6a19\u6e96\u3067\u3059\u304c\u3001\u8b1b\u5e2b\u306b\u3088\u3063\u3066\u306f\u5916\u56fd\u8a9e\uff08\u82f1\u8a9e\uff09\u3068\u306a\u308b\u5834\u5408\u304c\u3042\u308a\u307e\u3059\u3002\u8ac7\u8a71\u4f1a\u958b\u50ac\u3092\u5e0c\u671b\u3059\u308b\u65b9\u306f\u3001\u4e16\u8a71\u4eba\u307e\u3067\u3054\u9023\u7d61\u4e0b\u3055\u3044\u3002<\/p>\n<\/div>\n<\/div>\n

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  • 2011-15\u5e74\u5ea6\u3000\u534a\u7530 \u5229\u5f18\u3000Toshihiro Handa (2011-2015)<\/li>\n
  • 2016\u5e74\u5ea6\u3000\u00a0 \u00a0 \u00a0\u9ad8\u6851 \u7e41\u4e45\u3000Shigehisa Takakuwa (2016)<\/li>\n
  • 2017\u5e74\u5ea6\u3000\u00a0 \u00a0 \u00a0\u65b0\u6c38 \u6d69\u5b50\u3000Hiroko Shinnaga (2017)<\/li>\n
  • 2018\u5e74\u5ea6\u3000\u00a0 \u00a0 \u00a0\u4e2d\u897f \u88d5\u4e4b\u3000Hiroyuki Nakanishi (2018)<\/li>\n
  • 2019\u5e74\u5ea6\u3000\u00a0 \u00a0 \u00a0\u585a\u672c \u88d5\u4ecb\u3000Yusuke Tsukamoto (2019)<\/li>\n
  • 2021-22\u5e74\u5ea6\u00a0 \u00a0\u534a\u7530 \u5229\u5f18\u3000Toshihiro Handa (2021-2022)<\/li>\n
  • 2023\u5e74\u5ea6\u3000\u00a0 \u00a0 \u00a0\u585a\u672c \u88d5\u4ecb\u3000Yusuke Tsukamoto (2023)<\/li>\n
  • 2024\u5e74\u5ea6\u3000\u00a0 \u00a0 \u00a0\u8c37\u672c \u6566\u3000\u3000atsushi tanimoto (2024)<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n
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    \u8b1b\u6f14\u5c65\u6b74<\/h3>\n

    2026\u5e74\u5ea6<\/h4>\n\n\n\n
    \u7b2c147\u56de<\/td>\n2026\/4\/24<\/td>\nBenedikt Gottstein (\u30d9\u30eb\u30f3\u5927\u5b66)\u300cPlanetary formation tracks on the Hertzsprung\u2013Russell diagram\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2025\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c146\u56de<\/td>\n2026\/3\/17<\/td>\n\u9577\u5c3e \u5d07\u53f2 (\u56fd\u7acb\u5929\u6587\u53f0\/Truku\u5927\u5b66)\u300c\u91cd\u529b\u5d29\u58ca\u578b\u8d85\u65b0\u661f\u306e\u591a\u69d8\u306a\u7206\u767a\u5f62\u72b6\u304b\u3089\u63a2\u308b\u7206\u767a\u6a5f\u69cb\u300d<\/td>\n<\/tr>\n<\/tbody>\n
    \u7b2c145\u56de<\/td>\n2026\/3\/2<\/td>\nElizabeth Cappellazzo (Macquarie University \/ CSIRO Astronomy and Space Science)\u300cSurveying Interactions between HII regions and their Parent Molecular Clouds\u300d<\/td>\n<\/tr>\n<\/tbody>\n
    \u7b2c144\u56de<\/td>\n2026\/2\/19<\/td>\n\u5c71\u5ba4 \u826f\u592a (\u6771\u4eac\u79d1\u5b66\u5927\u5b66)\u300c\u5927\u8cea\u91cf\u539f\u59cb\u661f\u5186\u76e4\u306b\u304a\u3051\u308b\u30c0\u30b9\u30c8\u6210\u9577 : \u5ca9\u77f3\u30c0\u30b9\u30c8\u306e\u6210\u9577\u904e\u7a0b\u3078\u306e\u5236\u7d04\u300d<\/td>\n<\/tr>\n<\/tbody>\n
    \u7b2c143\u56de<\/td>\n2026\/2\/9<\/td>\nChang Liu (Sun Yat-sen University, China)\u300cTwo Sequences Appear in the 4 \u03bcm\u2013SiO Maser Flux Correlation for Circumstellar SiO Maser Sources\u300d<\/td>\n<\/tr>\n<\/tbody>\n
    \u7b2c142\u56de<\/td>\n2025\/11\/25<\/td>\n\u5ca9\u6fa4 \u4e00\u53f8 (University of Barcelona)\u300c\u30b9\u30bf\u30fc\u30d0\u30fc\u30b9\u30c8\u9280\u6cb3M82\u306e\u9ad8\u6e29\u30ac\u30b9\u3068\u9280\u6cb3\u98a8\u300d<\/td>\n<\/tr>\n<\/tbody>\n
    \u7b2c141\u56de<\/td>\n2025\/10\/16<\/td>\nBert Vander Meulen (European Space Agency)\u300cX-ray radiative transfer with the SKIRT code\u300d<\/td>\n<\/tr>\n<\/tbody>\n
    \u7b2c140\u56de<\/td>\n2025\/7\/3<\/td>\nI-Hsuan Kuo (University of Arizona)\u300cKinematical Signatures in the Protoplanetary Disk MWC 758\u300d<\/td>\n<\/tr>\n<\/tbody>\n
    \u7b2c139\u56de<\/td>\n2025\/4\/7<\/td>\nJoanne Dawson (Macquarie University\uff09\u300cSmall-scale structure of the Dark ISM\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2024\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c138\u56de<\/td>\n2025\/3\/26<\/td>\n\u5927\u6a4b \u6c38\u82b3 (\u53f0\u6e7e\u4e2d\u592e\u7814\u7a76\u9662\u5929\u4f53\u53ca\u5929\u4f53\u7269\u7406\u7814\u7a76\u6240\uff09\u300c\u30a2\u30eb\u30de\u304c\u89e3\u304d\u660e\u304b\u3059\u60d1\u661f\u5f62\u6210\u6700\u521d\u671f\u6bb5\u968e\u300d<\/td>\n<\/tr>\n
    \u7b2c137\u56de<\/td>\n2025\/2\/18<\/td>\n\u5e73\u677e \u6b63\u9855 (\u56fd\u7acb\u5929\u6587\u53f0 \u5929\u6587\u60c5\u5831\u30bb\u30f3\u30bf\u30fc\uff09\u300c\u5468\u6ce2\u6570\u8cc7\u6e90\u4fdd\u8b77\uff1a\u96fb\u6ce2\u5929\u6587\u5b66\u3068\u60c5\u5831\u901a\u4fe1\u793e\u4f1a\u306e\u5171\u5b58\u306b\u5411\u3051\u3066\u300d<\/td>\n<\/tr>\n
    \u7b2c136\u56de<\/td>\n2024\/12\/20<\/td>\nYueh-Ning Lee (Department of Earth Sciences, National Taiwan Normal University)\u300cHow nonideal magnetohydrodynamics regulates the formation and evolution of young protoplanetary disks\u300d<\/td>\n<\/tr>\n
    \u7b2c135\u56de<\/td>\n2024\/12\/20<\/td>\nYi-Jehng Kuan (Center of Astronomy and Gravitation, National Taiwan Normal University)\u300cMolecular Study of Icy Ocean Worlds\u300d<\/td>\n<\/tr>\n
    \u7b2c134\u56de<\/td>\n2024\/10\/9<\/td>\nIlseung Han (Seoul National University)\u300cFrom Dust to Planets: When Do Grains Grow in Disks?\u300d<\/td>\n<\/tr>\n
    \u7b2c133\u56de<\/td>\n2024\/9\/5<\/td>\n\u829d\u6c60 \u8aed\u4eba (\u56fd\u7acb\u5929\u6587\u53f0)\u300c\u5468\u60d1\u661f\u5186\u76e4\u306e\u30c0\u30b9\u30c8\u71b1\u653e\u5c04\u304b\u3089\u5236\u7d04\u3059\u308b\u5f62\u6210\u4e2d\u306e\u30ac\u30b9\u60d1\u661f\u306e\u7279\u6027\u300d<\/td>\n<\/tr>\n
    \u7b2c132\u56de<\/td>\n2024\/8\/12<\/td>\nChamani Gunasekera (University of Kentucky)\u300cPreparing for High-Resolution X-rays in the Microcalorimeter Era\u300d<\/td>\n<\/tr>\n
    \u7b2c131\u56de<\/td>\n2024\/8\/12<\/td>\nPeter van Hoof (Royal Observatory of Belgium)\u300cDust and molecules in PNe\u300d<\/td>\n<\/tr>\n
    \u7b2c130\u56de<\/td>\n2024\/6\/13<\/td>\n\u5c71\u53e3 \u6b63\u884c (Academia Sinica Institute of Astronomy and Astrophysics)\u300cALMA 2D super-resolution imaging of Taurus-Auriga protoplanetary disks: Probing statistical properties of disk substructures\u300d<\/td>\n<\/tr>\n
    \u7b2c129\u56de<\/td>\n2024\/5\/24<\/td>\nRoldan Cala (Instituto de Astrof\u00edsica de Andaluc\u00eda)\u300cH2O\/OH masers, `water fountains’, non-thermal radio continuum, and dual chemistry of nascent planetary nebulae\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2023\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c128\u56de<\/td>\n2024\/3\/4<\/td>\n\u9ad8\u6a4b \u5e79\u5f25 (\u7b51\u6ce2\u5927\u5b66)\u300c\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u306e\u89b3\u6e2c\u30a4\u30e1\u30fc\u30b8\u306b\u3088\u308b\u6642\u7a7a\u69cb\u9020\u306e\u63a8\u5b9a\u300d<\/td>\n<\/tr>\n
    \u7b2c127\u56de<\/td>\n2024\/3\/1<\/td>\n\u677e\u6728\u5834 \u4eae\u559c (\u4eac\u90fd\u5927\u5b66)\u300c\u539f\u59cb\u60d1\u661f\u7cfb\u5186\u76e4\u306e\u30ac\u30b9-\u30c0\u30b9\u30c82\u6210\u52062\u6b21\u5143\u30b0\u30ed\u30fc\u30d0\u30eb\u8a08\u7b97\u306b\u3088\u308b\u5186\u76e4\u9032\u5316\u3068\u30c0\u30b9\u30c8\u30ea\u30f3\u30b0\u5f62\u6210\u300d<\/td>\n<\/tr>\n
    \u7b2c126\u56de<\/td>\n2024\/2\/29<\/td>\nDr. Jayender Kumar (CSIRO Astronomy & Space Science)\u300cThe Structure and 3D Kinematics within 4 kpc of the Galactic Centre\u300d<\/td>\n<\/tr>\n
    \u7b2c125\u56de<\/td>\n2024\/2\/21<\/td>\n\u690d\u6751 \u8aa0 (\u5e83\u5cf6\u5927\u5b66)\u300c\u591a\u8272\u6e2c\u5149\u89b3\u6e2c\u306b\u3088\u308b\u6fc0\u5909\u661f\u306e\u7814\u7a76\u300d<\/td>\n<\/tr>\n
    \u7b2c124\u56de<\/td>\n2023\/12\/21<\/td>\n\u5ddd\u7aef \u5f18\u6cbb (\u5e83\u5cf6\u5927\u5b66)\u300c\u5e83\u5cf6\u5927\u304b\u306a\u305f\u671b\u9060\u93e1\u306e\u8fd1\u6cc1\u3068\u9280\u6cb3\u78c1\u5834\u30b5\u30fc\u30d9\u30a4\u89b3\u6e2c\u300d<\/td>\n<\/tr>\n
    \u7b2c123\u56de<\/td>\n2023\/12\/21<\/td>\n\u51a8\u6c38 \u671b (\u56fd\u7acb\u5929\u6587\u53f0)\u300cSupernovae, Multi-messenger astronomy, and Galactic archeology\u300d<\/td>\n<\/tr>\n
    \u7b2c122\u56de<\/td>\n2023\/12\/14<\/td>\nDevendra Sahu (Indian Institute of Astrophysics)\u300cSupernova studies at Indian Institute of Astrophysics\u300d<\/td>\n<\/tr>\n
    \u7b2c121\u56de<\/td>\n2023\/12\/4<\/td>\n\u5c0f\u9ad8\u88d5\u548c (\u5927\u962a\u5927\u5b66\u51c6\u6559\u6388)\u300cMonte Carlo radiative transfer code MONACO for X-ray astronomy—the framework design and its applications to molecular clouds, black holes, and neutron stars\u300d<\/td>\n<\/tr>\n
    \u7b2c120\u56de<\/td>\n2023\/11\/2<\/td>\n\u5cf0\u5d0e \u5cb3\u592b (\u6771\u4eac\u5927\u5b66\u5927\u5b66\u9662\u7406\u5b66\u7cfb\u7814\u7a76\u79d1\u9644\u5c5e\u5929\u6587\u5b66\u6559\u80b2\u7814\u7a76\u30bb\u30f3\u30bf\u30fc)\u300c\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u6642\u9593\u8ef8\u5929\u6587\u5b66\uff08time-domain study for AGNs\uff09\u300d<\/td>\n<\/tr>\n
    \u7b2c119\u56de<\/td>\n2023\/9\/8<\/td>\n\u5317\u5c71 \u54f2 (\u6771\u90a6\u5927\u5b66\u6559\u6388)\u300c\u30b9\u30cb\u30e4\u30a8\u30d5\u30fb\u30bc\u30eb\u30c9\u30d3\u30c3\u30c1\u52b9\u679c\u306e\u9ad8\u89e3\u50cf\u5ea6\u6e2c\u5b9a\u3067\u63a2\u308b\u9280\u6cb3\u56e3\u9032\u5316\u300d<\/td>\n<\/tr>\n
    \u7b2c118\u56de<\/td>\n2023\/6\/16<\/td>\nYen, Hsi-Wei (ASIAA \u526f\u7814\u7a76\u54e1)\u300cInfluence of Magnetic Fields on Protoplanetary Disk Formation and Evolution\u300d<\/td>\n<\/tr>\n
    \u7b2c117\u56de<\/td>\n2023\/5\/29<\/td>\n\u78ef\u8c9d \u6842\u4ecb (\u4eac\u90fd\u5927\u5b66\u5ca1\u5c71\u5929\u6587\u53f0\u7279\u5b9a\u52a9\u6559)\u300c\u53ef\u8996\u6e2c\u5149\u30fb\u5206\u5149\u89b3\u6e2c\u306b\u3088\u308b\u6fc0\u5909\u661f\u306e\u964d\u7740\u5186\u76e4\u6d3b\u52d5\u73fe\u8c61\u306e\u89e3\u660e\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2022\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c116\u56de<\/td>\n2023\/3\/31<\/td>\nTatiana M. Rodriguez (New Mexico Institute of Mining and Technology)\u300cA multiscale approach to understand outflows from high-mass protostars\u300d<\/td>\n<\/tr>\n
    \u7b2c115\u56de<\/td>\n2023\/3\/27<\/td>\n\u5927\u6edd \u6052\u8f1d (\u7b51\u6ce2\u5927\u5b66)\u300c\u30b5\u30d6\u30cf\u30ed\u30fc\u885d\u7a81\u3068\u77ee\u5c0f\u9280\u6cb3\u306e\u5f62\u6210\u904e\u7a0b\u300d<\/td>\n<\/tr>\n
    \u7b2c114\u56de<\/td>\n2023\/3\/27<\/td>\n\u5927\u5c0f\u7530 \u7d50\u8cb4 (\u7406\u5316\u5b66\u7814\u7a76\u6240)\u300c\u6700\u521d\u671f\u5f62\u6210\u904e\u7a0b\u306b\u304a\u3051\u308b\u4f4e\u8cea\u91cf\u539f\u59cb\u661f\u5929\u4f53\u306e\u7269\u7406\u69cb\u9020\u300d<\/td>\n<\/tr>\n
    \u7b2c113\u56de<\/td>\n2023\/3\/9<\/td>\n\u67ff\u5185 \u5065\u4f51 (\u540d\u53e4\u5c4b\u5927\u5b66)\u300cEnergetics and Dynamics of Interstellar Gas Disks Affected by Magnetic Activity in the Galactic Bulge Region\u300d<\/td>\n<\/tr>\n
    \u7b2c112\u56de<\/td>\n2023\/3\/3<\/td>\nYik Ki (Jackie) Ma (Australian National University)\u300cPotential HI Compass Needles in the Small Magellanic Cloud?\u300d<\/td>\n<\/tr>\n
    \u7b2c111\u56de<\/td>\n2023\/2\/6<\/td>\n\u8863\u5ddd \u667a\u5f25 (\u6771\u4eac\u5927\u5b66)\u300c\u5b87\u5b99\u521d\u671f\u5929\u4f53\u304b\u3089\u306e\u91cd\u529b\u6ce2\u300d<\/td>\n<\/tr>\n
    \u7b2c110\u56de<\/td>\n2023\/1\/24<\/td>\n\u9808\u85e4 \u9756 (\u6771\u4eac\u5927\u5b66)\u300c\u968e\u5c64\u7684\u4e09\u4f53\u7cfb\u306e\u529b\u5b66\u7684\u5b89\u5b9a\u6027\u3068ZKL\u52b9\u679c\u300d<\/td>\n<\/tr>\n
    \u7b2c109\u56de<\/td>\n2023\/1\/10<\/td>\n\u9ad8\u6a4b \u5b9f\u9053 (\u56fd\u7acb\u5929\u6587\u53f0)\u300c\u539f\u59cb\u60d1\u661f\u7cfb\u5186\u76e4\u4e2d\u306e\u30c0\u30b9\u30c8\u30ea\u30f3\u30b0\u69cb\u9020\u306e\u91cd\u529b\u5d29\u58ca\u306b\u3088\u308b\u5fae\u60d1\u661f\u5f62\u6210\u300d<\/td>\n<\/tr>\n
    \u7b2c108\u56de<\/td>\n2022\/12\/13<\/td>\n\u5c71\u4e2d \u96c5\u4e4b (\u9e7f\u5150\u5cf6\u5927\u5b66\u5929\u306e\u5ddd\u9280\u6cb3\u7814\u7a76\u30bb\u30f3\u30bf\u30fc)\u300c\u8fd1\u8d64\u5916\u7dda\u89b3\u6e2c\u3067\u8feb\u308b\u8d85\u65b0\u661f\u3068\u7a81\u767a\u73fe\u8c61\u300d<\/td>\n<\/tr>\n
    \u7b2c107\u56de<\/td>\n2022\/11\/29<\/td>\nPatrick Woudt (University of Cape Town)\u300cMeerKAT and MeerLICHT: A New Look at Radio Transients\u300d<\/td>\n<\/tr>\n
    \u7b2c106\u56de<\/td>\n2022\/11\/24<\/td>\nPatrick Woudt (University of Cape Town)\u300cV445 Puppis – a unique helium nova\u300d<\/td>\n<\/tr>\n
    \u7b2c105\u56de<\/td>\n2022\/11\/22<\/td>\nKin Hang (Paul) YEUNG (\u6771\u4eac\u5927\u5b66\u7406\u5b66\u90e8)\u300cMultiwavelength studies of G298.6-0.0: Possibly one of the oldest GeV supernova remnants\u300d<\/td>\n<\/tr>\n
    \u7b2c104\u56de<\/td>\n2022\/11\/18<\/td>\nJosep M. Girart (Institute of Space Sciences)\u300cThe ALMA view of the role of the magnetic fields in star formation process\u300d<\/td>\n<\/tr>\n
    \u7b2c103\u56de<\/td>\n2022\/11\/14<\/td>\n\u670d\u90e8 \u516c\u5e73 (\u56fd\u7acb\u5929\u6587\u53f0)\u300c\u6052\u661f\u30cf\u30ed\u30fc\u306e\u904b\u52d5\u60c5\u5831\u3067\u63a2\u308b\u9280\u6cb3\u7cfb\u306e\u69cb\u9020\u3068\u5f62\u6210\u53f2\u300d<\/td>\n<\/tr>\n
    \u7b2c102\u56de<\/td>\n2022\/9\/27<\/td>\n\u6d45\u5c71 \u4fe1\u4e00\u90ce (Square Kilometre Array Observatory)\u300cSKA1\u30b7\u30b9\u30c6\u30e0\u6982\u8981\u3068\u79d1\u5b66\u7684\u8a55\u4fa1\u8a66\u9a13\u300d<\/td>\n<\/tr>\n
    \u7b2c101\u56de<\/td>\n2022\/9\/ 6<\/td>\n\u5cf6\u5c3b \u82b3\u4eba (\u56fd\u7acb\u5929\u6587\u53f0)\u300c\u6a5f\u68b0\u5b66\u7fd2\u306b\u3088\u308b\u5206\u5b50\u8f1d\u7dda\u30c7\u30fc\u30bf\u304b\u3089\u306eH2\u67f1\u5bc6\u5ea6\u5206\u5e03\u306e\u4e88\u6e2c\u300d<\/td>\n<\/tr>\n
    \u7b2c100\u56de<\/td>\n2022\/8\/17<\/td>\nDaniel Espada (Granada university)\u300c Unveiling the Multiphase Gas Properties and SF Laws around the closest radio powerful AGN, Centaurus A\u300d<\/td>\n<\/tr>\n
    \u7b2c99\u56de<\/td>\n2022\/5\/26<\/td>\n\u524d\u7530 \u90c1\u5f25 (\u6771\u4eac\u5927\u5b66\u5929\u6587\u5b66\u6559\u80b2\u7814\u7a76\u30bb\u30f3\u30bf\u30fc)\u300c\u68d2\u6e26\u5dfb\u9280\u6cb3\u306b\u304a\u3051\u308b\u661f\u5f62\u6210\u6291\u5236\u30e1\u30ab\u30cb\u30ba\u30e0\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2021\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n
    \u7b2c98\u56de<\/td>\n2021\/12\/20<\/td>\n\u77e2\u5cf6 \u7fa9\u4e4b(\u5317\u6d77\u9053\u5927\u5b66 \u5f8c\u671f\u535a\u58eb\u8ab2\u7a0b3\u5e74)\u300c\u8fd1\u508d\u9280\u6cb3\u306e low-J CO \u89b3\u6e2c\u306b\u3088\u308b\u5206\u5b50\u30ac\u30b9\u306e\u7269\u7406\u72b6\u614b\u300d<\/td>\n<\/tr>\n
    \u7b2c97\u56de<\/td>\n2021\/12\/15<\/td>\n\u5bcc\u962a \u5e78\u6cbb(\u56fd\u7acb\u5929\u6587\u53f0\u540d\u8a89\u6559\u6388)\u300c\u661f\u5f62\u6210\u306b\u304a\u3051\u308b\u78c1\u5834\u306e\u5f79\u5272—\u30a2\u30a6\u30c8\u30d5\u30ed\u30fc\u3001\u30d5\u30a3\u30e9\u30e1\u30f3\u30c8\u3001\u504f\u5149\uff08\u504f\u6ce2\uff09\u306b\u7740\u76ee\u3057\u3066\u300d<\/td>\n<\/tr>\n
    \u7b2c96\u56de<\/td>\n2021\/12\/10<\/td>\n\u6cc9 \u62d3\u78e8 (\u56fd\u7acb\u5929\u6587\u53f0)\u300c\u3059\u3070\u308b\u3068ALMA\u3067\u6311\u3080\u9280\u6cb3\u3068\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u306e\u59cb\u539f\u7684\u5171\u9032\u5316\u300d<\/td>\n<\/tr>\n
    \u7b2c95\u56de<\/td>\n2021\/12\/8<\/td>\n\u897f\u5408 \u4e00\u77e2 (\u6771\u4eac\u5927\u5b66\u7406\u5b66\u7814\u7a76\u79d1)\u300c\u539f\u59cb\u661f\u5929\u4f53\u306e\u529b\u5b66\u69cb\u9020\u304c\u793a\u3059\u591a\u69d8\u306a\u661f\u5f62\u6210\u74b0\u5883\u306e\u89e3\u660e\u300d<\/td>\n<\/tr>\n
    \u7b2c94\u56de<\/td>\n2021\/11\/25<\/td>\n\u9577\u5c3e \u900f (\u611b\u5a9b\u5927\u5b66\u5b87\u5b99\u9032\u5316\u7814\u7a76\u30bb\u30f3\u30bf\u30fc\u6559\u6388)\u300c\u3059\u3070\u308bHSC\u3067\u898b\u305f\u96fb\u6ce2\u9280\u6cb3\u300d<\/td>\n<\/tr>\n
    \u7b2c93\u56de<\/td>\n2021\/11\/12<\/td>\n\u9152\u898b \u306f\u308b\u9999 (\u9e7f\u5150\u5cf6\u5927\u5b66\u30d7\u30ed\u30b8\u30a7\u30af\u30c8\u7814\u7a76\u54e1)\u300c\u30de\u30a4\u30af\u30ed\u30af\u30a8\u30fc\u30b5\u30fcSS433\u306e\u30b8\u30a7\u30c3\u30c8\u306b\u3088\u308b\u5b87\u5b99\u7dda\u7c92\u5b50\u52a0\u901f\u300d<\/td>\n<\/tr>\n
    \u7b2c92\u56de<\/td>\n2021\/10\/ 22<\/td>\n\u99ac\u5834 \u4fca\u4ecb (\u9e7f\u5150\u5cf6\u5927\u5b66\u30d7\u30ed\u30b8\u30a7\u30af\u30c8\u7814\u7a76\u54e1)\u300c\u8d64\u5916\u7dda\u3068\u30b5\u30d6\u30df\u30ea\u6ce2\u3067\u63a2\u308b\u8d85\u9ad8\u5149\u5ea6\u8d64\u5916\u7dda\u9280\u6cb3\u306e\u71b1\u6e90\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2020\u5e74\u5ea6<\/h4>\n\n\n\n\n
    \u7b2c91\u56de<\/td>\n2021\/1\/18<\/td>\n\u6751\u702c \u5efa (\u9e7f\u5150\u5cf6\u5927\u5b66\u7406\u5de5\u5b66\u7814\u7a76\u79d1 \u5f8c\u671f\u535a\u58eb\u8ab2\u7a0b1\u5e74)\u300c\u8907\u6570\u306e\u7570\u306a\u308b\u5206\u5b50\u8f1d\u7dda\u3092\u7528\u3044\u305f\u661f\u9593\u30ac\u30b9\u96f2\u306e\u7279\u6027\u300d<\/td>\n<\/tr>\n
    \u7b2c90\u56de<\/td>\n2020\/10\/ 6<\/td>\nRoss A. Burns (EACOA, NAOJ, KASI)\u300cRecent findings of the Maser Monitoring Organisation (M2O)\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2019\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c89\u56de<\/td>\n2020\/3\/30<\/td>\n\u5409\u7530 \u96c4\u57ce\uff08\u56fd\u7acb\u5929\u6587\u53f0\u79d1\u5b66\u7814\u7a76\u90e8\uff09\u300c\u6e26\u72b6\u8155\u5f62\u6210\u306e\u7d20\u904e\u7a0b\u300d<\/td>\n<\/tr>\n
    \u7b2c88\u56de<\/td>\n2020\/1\/31<\/td>\nRhona Hamilton (\u30a2\u30c7\u30ec\u30fc\u30c9\u5927\u5b66)\u3000\u300cA multifrequency study of the M87 jet\u300d<\/td>\n<\/tr>\n
    \u7b2c87\u56de<\/td>\n2020\/1\/30<\/td>\n\u7530\u6751 \u967d\u4e00 \uff08\u540d\u53e4\u5c4b\u5927\u5b66\uff09\u300c\u30b5\u30d6\u30df\u30ea\u6ce2\u89b3\u6e2c\u3067\u3055\u3050\u308b\u5b87\u5b99\u306e\u591c\u660e\u3051\u3068\u9280\u6cb3\u306e\u8a95\u751f\u300d<\/td>\n<\/tr>\n
    \u7b2c86\u56de<\/td>\n2019\/12\/23<\/td>\n\u5e78\u7530 \u4ec1 (\u30cb\u30e5\u30fc\u30e8\u30fc\u30af\u5dde\u7acb\u5927\u5b66\u30b9\u30c8\u30fc\u30cb\u30fc\u30d6\u30eb\u30c3\u30af\u6821)\u3000\u300c\u8fd1\u508d\u9280\u6cb3\u3068\u9280\u6cb3\u7cfb\u306e\u661f\u9593\u30ac\u30b9\u3001\u661f\u5f62\u6210\u3001\u69cb\u9020\u306a\u3069\u300d<\/td>\n<\/tr>\n
    \u7b2c85\u56de<\/td>\n2019\/12\/20<\/td>\n\u4e8c\u9593\u702c \u654f\u53f2\uff08\u4eac\u90fd\u7523\u696d\u5927\u5b66\uff09\u300c\u30a2\u30a4\u30f3\u30b7\u30e5\u30bf\u30a4\u30f3\u65b9\u7a0b\u5f0f\u306e\u5e73\u5747\u5316\u3068\u30cf\u30c3\u30d6\u30eb\u5b9a\u6570\u554f\u984c\u306e\u89e3\u6c7a\u6cd5\u300d<\/td>\n<\/tr>\n
    \u7b2c84\u56de<\/td>\n2019\/ 11\/ 1<\/td>\nDr. Marc Schartmann(Excellence Cluster Origins Ludwig-Maximilians-Universit\u00e4t & MPE)\u300cThe life cycle of circumnuclear gas discs in nearby galactic nuclei\u300d<\/td>\n<\/tr>\n
    \u7b2c83\u56de<\/td>\n2019\/ 9\/ 24<\/td>\n\u798f\u4e95 \u5eb7\u96c4(\u540d\u53e4\u5c4b\u5927\u5b66)\u300cActive star formation from HI gas in galaxies\u300d<\/td>\n<\/tr>\n
    \u7b2c82\u56de<\/td>\n2019\/ 9\/ 19<\/td>\nEduardo de la Fuente Acosta (Physics Department, CUCEI, Universidad de Guadalajara and CONACyT “HAWC” National Laboratory)\u300c\u661f\u5f62\u6210\u9818\u57df\u306b\u5bfe\u3059\u308b\u03b3\u7dda\u304b\u3089\u96fb\u6ce2\u306b\u308f\u305f\u308b\u591a\u6ce2\u9577\u3067\u306e\u89b3\u6e2c\u300d<\/td>\n<\/tr>\n
    \u7b2c81\u56de<\/td>\n2019\/ 8\/ 1<\/td>\nPierre Marchand (\u5927\u962a\u5927\u5b66)\u300cAngular momentum regulation in star formation\u300d<\/td>\n<\/tr>\n
    \u7b2c80\u56de<\/td>\n2019\/ 8\/ 1<\/td>\n\u7530\u4e2d \u572d(\u5927\u962a\u5927\u5b66) \u300c\u5927\u8cea\u91cf\u661f\u5f62\u6210\u306b\u304a\u3051\u308b\u8907\u5408\u30d5\u30a3\u30fc\u30c9\u30d0\u30c3\u30af\u300d<\/td>\n<\/tr>\n
    \u7b2c79\u56de<\/td>\n2019\/ 7\/22<\/td>\n\u5fb3\u7530 \u4e00\u8d77 (\u5927\u962a\u5e9c\u7acb\u5927\u5b66) \u300cALMA\u306b\u3088\u308b\u5c0f\u8cea\u91cf\u661f\u5f62\u6210\u9818\u57df\u5206\u5b50\u96f2\u30b3\u30a2\u306e\u8a73\u7d30\u89b3\u6e2c\u300d<\/span><\/td>\n<\/tr>\n
    \u7b2c78\u56de<\/td>\n2019\/ 7\/18<\/td>\n\u5824\u5927\u9678 (\u540d\u53e4\u5c4b\u5927\u5b66) \u300c\u30aa\u30ea\u30aa\u30f3\u5ea7\u5206\u5b50\u96f2\u306b\u304a\u3051\u308b\u5927\u8cea\u91cf\u661f\u5f62\u6210\u3068\u8d85\u5e83\u57df\u5206\u5b50\u96f2\u30b5\u30fc\u30d9\u30a4NASCO\u300d<\/td>\n<\/tr>\n
    \u7b2c77\u56de<\/td>\n2019\/ 7\/16<\/td>\nLech Wiktor Piotrowski (\u7406\u5316\u5b66\u7814\u7a76\u6240) \u300cOptical observations of heavy stable macro particles crossing the atmosphere<\/span>\u300d<\/span><\/td>\n<\/tr>\n
    \u7b2c76\u56de<\/td>\n2019\/ 6\/ 3<\/td>\n\u585a\u8d8a\u5d07\uff08\u56fd\u7acb\u5929\u6587\u53f0 \u7279\u4efb\u6559\u6388\uff09\u300cALMA\u3067\u63a2\u308bTWHya\u3092\u53d6\u308a\u5dfb\u304f\u539f\u59cb\u60d1\u661f\u7cfb\u5186\u76e4\u306e\u8a73\u7d30\u69cb\u9020\u300d<\/td>\n<\/tr>\n
    \u7b2c75\u56de<\/td>\n2019\/ 5\/29<\/td>\n\u5cf6\u5c3b\u82b3\u4eba\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\/\u56fd\u7acb\u5929\u6587\u53f0\uff09\u300c\u30d5\u30a3\u30e9\u30e1\u30f3\u30c8\u5f62\u6210\u30b7\u30ca\u30ea\u30aa\u306e\u666e\u904d\u6027 –\u5927\u8cea\u91cf\u661f\u5f62\u6210\u9818\u57df\u306b\u304a\u3051\u308b\u30d5\u30a3\u30e9\u30e1\u30f3\u30c8\u5f62\u6210–\u300d<\/td>\n<\/tr>\n
    \u7b2c74\u56de<\/td>\n2019\/ 5\/21<\/td>\n\u5c71\u5185\u6b63\u5247\u535a\u58eb\uff08\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u52a0\u901f\u5668\u7814\u7a76\u6a5f\u69cb \u6a5f\u69cb\u9577\uff09\u300c\u52a0\u901f\u5668\u306b\u3088\u308b\u7d20\u7c92\u5b50\u7814\u7a76\u300d<\/td>\n<\/tr>\n
    \u7b2c73\u56de<\/td>\n2019\/ 5\/10<\/td>\nColin Norman\uff08John Hopkins University\uff09\u300cHigh Redshift Quasars: Formation, Feedback and Environment\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2018\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c72\u56de<\/td>\n2019\/ 3\/19<\/td>\n\u85e4\u672c\u88d5\u8f14\uff08\u30aa\u30fc\u30b9\u30c8\u30e9\u30ea\u30a2\u56fd\u7acb\u5927\u5b66\uff09\u300c\u9280\u6cb3\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u3067\u63a2\u308b\u3001\u5206\u5b50\u96f2\u5f62\u6210\u3068\u9032\u5316\u3001\u661f\u5f62\u6210\u3001\u305d\u3057\u3066\u9280\u6cb3\u7cfb\u306b\u304a\u3051\u308b\u592a\u967d\u7cfb\u306e\u5f62\u6210\u74b0\u5883\u300d<\/td>\n<\/tr>\n
    \u7b2c71\u56de<\/td>\n2019\/ 2\/28<\/td>\n\u5927\u7530\u3000\u6cc9\uff08\u7532\u5357\u5927\u5b66\uff09\u300c\u30c6\u30e9\u30d8\u30eb\u30c4\u5e2f\u6642\u9593\u9818\u57df\u5206\u5149\u6cd5\u3092\u7528\u3044\u305f\u5149\u5b66\u7d20\u5b50\u306e\u4e8c\u6b21\u5143\u9762\u5185\u7a7a\u9593\u5206\u89e3\u53ef\u80fd\u306a\u5206\u5149\u8a55\u4fa1\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\u300d<\/td>\n<\/tr>\n
    \u7b2c70\u56de<\/td>\n2019\/ 2\/22<\/td>\n\u5cf6\u888b\u96bc\u58eb\uff08\u4e2d\u56fd\uff1a\u6e05\u83ef\u5927\u5b66\uff09\u300c\uff12\uff11cm\u7dda\u3067\u63a2\u308b\u5b87\u5b99\u518d\u96fb\u96e2\u671f\u300d<\/td>\n<\/tr>\n
    \u7b2c69\u56de<\/td>\n2018\/12\/12<\/td>\n\u99ac\u5d8b\u79c0\u884c\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\u533b\u6b6f\u5b66\u7dcf\u5408\u7814\u7a76\u79d1\uff09\u300c\u6bdb\u9aea\u306b\u5bfe\u3059\u308b\u5b87\u5b99\u653e\u5c04\u7dda\u5f71\u97ff\u7814\u7a76\u300d<\/td>\n<\/tr>\n
    \u7b2c68\u56de<\/td>\n2018\/11\/ 2<\/td>\n\u5cf6\u5c3b\u82b3\u4eba\uff08\u30b5\u30af\u30ec\u30fc\u539f\u5b50\u529b\u5e81\u30bb\u30f3\u30bf\u30fc\u3001\u30d5\u30e9\u30f3\u30b9\uff09\u300c\u96fb\u6ce2\u89b3\u6e2c\u304c\u660e\u3089\u304b\u306b\u3059\u308b\u661f\u5f62\u6210\u306e\u73fe\u5834\u300d<\/td>\n<\/tr>\n
    \u7b2c67\u56de<\/td>\n2018\/10\/10<\/td>\nWako Ishibashi (the Institute of Astronomy, University of Cambridge)\u300cThe role(s) of AGN radiative feedback in galaxy evolution\u300d<\/td>\n<\/tr>\n
    \u7b2c66\u56de<\/td>\n2018\/ 8\/23<\/td>\n\u753a\u7530\u3000\u771f\u7f8e (\u4e5d\u5dde\u5927\u5b66)\u300c\u6e26\u72b6\u9280\u6cb3\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u3092\u7528\u3044\u305f100MHz\uff5e10GHz\u5e2f\u306e\u64ec\u4f3c\u89b3\u6e2c\u300d<\/td>\n<\/tr>\n
    \u7b2c65\u56de<\/td>\n2018\/ 8\/23<\/td>\n\u5ddd\u908a\u826f\u5e73(\u56fd\u7acb\u5929\u6587\u53f0)\u30fb\u6cb3\u91ce\u5b5d\u592a\u90ce\uff08\u6771\u4eac\u5927\u5b66\uff09\u300c\u5927\u578b\u30b5\u30d6\u30df\u30ea\u6ce2\u671b\u9060\u93e1 LST\u300d<\/td>\n<\/tr>\n
    \u7b2c64\u56de<\/td>\n2018\/ 6\/28<\/td>\n\u6a2a\u5c71\u3000\u5e83\u7f8e (\u6771\u4eac\u5927\u5b66 Kavli IPMU)\u300c\u79d1\u5b66\u8005\u306e\u4fe1\u983c\u300d<\/td>\n<\/tr>\n
    \u7b2c63\u56de<\/td>\n2018\/ 6\/5<\/td>\nChikaedu Ogbodo (Macquarie University, Australia) \u300cPolarimetry of 1720-MHz OH Masers in Southern Star Forming Regions\u300d<\/td>\n<\/tr>\n
    \u7b2c62\u56de<\/td>\n2018\/ 6\/28<\/td>\n\u677e\u6d66\u3000\u664b\u4e5f (\u79d1\u5b66\u30b8\u30e3\u30fc\u30ca\u30ea\u30b9\u30c8)\u300c\u79d1\u5b66\u30b8\u30e3\u30fc\u30ca\u30ea\u30b9\u30c8\u3068\u3057\u3066\u306e\u7d4c\u9a13\u304b\u3089\uff08\u4eee\uff09\u300d<\/td>\n<\/tr>\n
    \u7b2c61\u56de<\/td>\n2018\/ 6\/ 1<\/td>\n\u4e8c\u9593\u702c\u654f\u53f2\uff08\u4eac\u90fd\u7523\u696d\u5927\u5b66\uff09\u300c\u30bf\u30a4\u30d7Ia\u578b\u8d85\u65b0\u661f\u306em-z\u95a2\u4fc2\u306e\u30ec\u30f3\u30ba\u52b9\u679c\u3068\u3001\u305d\u308c\u306b\u3088\u308b\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u8cea\u91cf\u3001\u30c0\u30fc\u30af\u30a8\u30cd\u30eb\u30ae\u30fc\u306e\u5236\u9650\u300d<\/td>\n<\/tr>\n
    \u7b2c60\u56de<\/td>\n2018\/ 4\/20<\/td>\nJose Maria Torrelles (Institut de Ciencies de l\u2019Espai, Barcelona)\u300cSome breakthroughs in the study of massive star formation through multi-epoch VLBI maser observations\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2017\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c59\u56de<\/td>\n2018\/ 3\/ 9<\/td>\nGabor Orosz (Xinjiang Astronomical Observatory, Chinese Academy of Sciences)
    \n\u300cEpisodic water fountain jets\u300d<\/td>\n<\/tr>\n
    \u7b2c58\u56de<\/td>\n2018\/ 2\/28<\/td>\nVachail Nicolas Salinas Poblete (Kagoshima University)\u300cDust evolution and chemistry in planet-forming disks\u300d<\/td>\n<\/tr>\n
    \u7b2c57\u56de<\/td>\n2018\/ 1\/23<\/td>\n\u9577\u5c3e\u3000\u900f (\u611b\u5a9b\u5927\u5b66\u5b87\u5b99\u9032\u5316\u7814\u7a76\u30bb\u30f3\u30bf\u30fc)\u300c\u3059\u3070\u308b\u671b\u9060\u93e1HSC\u3092\u7528\u3044\u305f\u5de8\u5927\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u9032\u5316\u306e\u7814\u7a76\u300d<\/td>\n<\/tr>\n
    \u7b2c56\u56de<\/td>\n2017\/12\/19<\/td>\n\u9234\u6728\u5efa (\u6771\u5927\u7dcf\u5408\u6587\u5316\/\u540d\u5927\u7406),\u67ff\u5185\u5065\u4f51 (\u540d\u5927\u7406\/\u6771\u5927\u7dcf\u5408\u6587\u5316)\u300c\u9280\u6cb3\u7cfb\u4e2d\u5fc3\u9818\u57df\u3067\u306e\u78c1\u6c17\u6d3b\u52d5\u3068\u30ac\u30b9\u306e\u52d5\u529b\u5b66\u300d<\/td>\n<\/tr>\n
    \u7b2c55\u56de<\/td>\n2017\/10\/ 6<\/td>\nSusanne Aalto (CHALMERS UNIVERSITY OF TECHNOLOGY Sweden)\u300cMolecular outflows in AGNs and starbursts\u300d<\/td>\n<\/tr>\n
    \u7b2c54\u56de<\/td>\n2017\/ 9\/28<\/td>\nKatherine M Pattle (University of Central Lancashire, U.K.)\u300cThe magnetic field strength and energetics of OMC 1\u300d<\/td>\n<\/tr>\n
    \u7b2c53\u56de<\/td>\n2017\/ 8\/24<\/td>\n\u5ddd\u52dd\u671b\uff08\u5449\u5de5\u696d\u9ad8\u7b49\u5c02\u9580\u5b66\u6821\uff09\u300c\u8d85\u65b0\u661f\u7206\u767a\u99c6\u52d5\u30e2\u30c7\u30eb\u306b\u3088\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u906e\u853d\u69cb\u9020\u300d<\/td>\n<\/tr>\n
    \u7b2c52\u56de<\/td>\n2017\/ 7\/12<\/td>\n\u5de5\u85e4\u7950\u5df1\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\u7406\u5b66\u90e8\u7269\u7406\u79d1\u5b66\u79d1\u548c\u7530\u7814\uff09\u300c\u5b87\u5b99\u7dda\u3092\u8003\u616e\u3057\u305f\u78c1\u6c17\u6d41\u4f53\u65b9\u7a0b\u5f0f\u306e\u65b0\u305f\u306a\u6570\u5024\u89e3\u6cd5\u300d<\/td>\n<\/tr>\n
    \u7b2c51\u56de<\/td>\n2017\/ 6\/28<\/td>\n\u7530\u4e2d\u3000\u6075\u7406\u5b50\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\u6570\u7406\u60c5\u5831\u79d1\u5b66\u5c02\u653b\uff09\u300c\u76f8\u5bfe\u8ad6\u7684\u5b8c\u5168\u6d41\u4f53\u306e\u5e7e\u4f55\u5b66\u7684\u5909\u5206\u539f\u7406\u300d<\/td>\n<\/tr>\n
    \u7b2c50\u56de<\/td>\n2017\/ 6\/26<\/td>\nAidan McGirr\uff08Arizona State University\uff09\u300cThe TeamIndus Lab2Moon Challenge and the viability of producing and developing Cube-Satellites\u300d<\/td>\n<\/tr>\n
    \u7b2c49\u56de<\/td>\n2017\/ 6\/13<\/td>\n\u620e\u5d0e\u4fca\u4e00\uff08\u7406\u5316\u5b66\u7814\u7a76\u6240\uff09\u300c\u30bf\u30f3\u30c7\u30e0\u60d1\u661f\u5f62\u6210\u7406\u8ad6\u306b\u3088\u308b\u5730\u7403\u306e\u8d77\u6e90\u300d<\/td>\n<\/tr>\n
    \u7b2c48\u56de<\/td>\n2017\/ 6\/7<\/td>\n\u7530\u4e2d\u4f51\u5e0c\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\u7406\u5b66\u90e8\u7269\u7406\u79d1\u5b66\u79d1\u585a\u672c\u7814\uff09\u300c\u78c1\u6c17\u6d41\u4f53\u6ce2\u52d5\u304c\u99c6\u52d5\u3059\u308b\u77ed\u5468\u671f\u30ac\u30b9\u60d1\u661f\u304b\u3089\u306e\u5927\u6c17\u6563\u9038\u3068\u9ad8\u5c64\u5927\u6c17\u69cb\u9020\u300d<\/td>\n<\/tr>\n
    \u7b2c47\u56de<\/td>\n2017\/ 5\/30<\/td>\n\u85e4\u7530\u3000\u88d5\uff08\u5927\u962a\u5927\u5b66\u5b87\u5b99\u5730\u7403\u79d1\u5b66\u5c02\u653b\uff09\u300c\u3072\u3068\u307f\u304c\u907a\u3057\u305f\u3082\u306e\u2015\u9280\u6cb3\u56e3\u52a0\u71b1\u6e90\u306e\u624b\u304c\u304b\u308a\u30fc\u300d<\/td>\n<\/tr>\n
    \u7b2c46\u56de<\/td>\n2017\/ 5\/25<\/td>\n\u971c\u7530\u3000\u6cbb\u6717\uff08\u9752\u5c71\u5b66\u9662\u5927\u5b66\u7406\u5de5\u5b66\u7814\u7a76\u79d1\uff09\u300c\u8d85\u65b0\u661f\u6b8b\u9ab8\u3067\u306e\u4e71\u6d41\u78c1\u5834\u30b9\u30da\u30af\u30c8\u30eb\u6307\u6570\u306e\u6e2c\u5b9a\u306b\u3064\u3044\u3066\u300d<\/td>\n<\/tr>\n
    \u7b2c45\u56de<\/td>\n2017\/ 5\/10<\/td>\n\u65b0\u6c38\u3000\u6d69\u5b50\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\u7269\u7406\u79d1\u5b66\u79d1\uff09\u300c\u7c73\u56fd\u56fd\u7acb\u96fb\u6ce2\u5929\u6587\u53f0\u30bd\u30b3\u30ed\u30ad\u30e3\u30f3\u30d1\u30b9\u3067\u306e\u6d77\u5916\u7814\u4fee \u2014 \u82e5\u624b\u6559\u54e1\u6d77\u5916\u7814\u4fee\u5831\u544a\u30fc\u300d<\/td>\n<\/tr>\n
    \u7b2c44\u56de<\/td>\n2017\/ 4\/25<\/td>\nColin Norman (Johns Hopkins University)\u300cThe formation and evolution of active galaxies and radio galaxies\u300d<\/td>\n<\/tr>\n
    \u7b2c43\u56de<\/td>\n2017\/ 4\/24<\/td>\nKohji Tomisaka (National Astronomical Observatory of Japan Theoretical Group)\u300cMagnetohydrostatic Structures of Magnetically-Supported Filaments and their Stability\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2016\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c42\u56de<\/td>\n2017\/ 3\/28<\/td>\nJamie Farnes\uff08Excellence Fellow, Radboud University Nijmegen)\u300cSeeing the Invisible Magnetic Universe\u300d<\/td>\n<\/tr>\n
    \u7b2c41\u56de<\/td>\n2017\/ 3\/21<\/td>\nPedro Russo\uff08\u30aa\u30e9\u30f3\u30c0\u30e9\u30a4\u30c7\u30f3\u5927\u5b66\u51c6\u6559\u6388,\u56fd\u969b\u5929\u6587\u5b66\u9023\u5408 Communicating Astronomy for Public[\u5927\u8846\u3068\u306e\u4ea4\u6d41\u304c\u3042\u308b\u5929\u6587\u5b66]\u5206\u79d1\u4f1a\u4f1a\u9577\uff09\u300cGlobal Programmes in Astronomy Education and Public Outreach[\u8a33]\u300c\u5929\u6587\u6559\u80b2\u666e\u53ca\u6d3b\u52d5\u306b\u304a\u3051\u308b\u4e16\u754c\u7684\u53d6\u7d44\u306b\u3064\u3044\u3066\u300d\u300d<\/td>\n<\/tr>\n
    \u7b2c40\u56de<\/td>\n2017\/ 3\/ 1<\/td>\n\u585a\u672c\u88d5\u4ecb\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\uff09\u300c\u30db\u30fc\u30eb\u52b9\u679c\u306b\u3088\u308b\u539f\u59cb\u60d1\u661f\u7cfb\u5186\u76e4\u306e\u5206\u5316\u9032\u5316\u3068Class 0\/I\u539f\u59cb\u60d1\u661f\u7cfb\u5186\u76e4\u4e2d\u3067\u306e\u30c0\u30b9\u30c8\u6210\u9577\u904e\u7a0b\u306e\u7814\u7a76\u300d<\/td>\n<\/tr>\n
    \u7b2c39\u56de<\/td>\n2017\/ 2\/ 8<\/td>\n\u91d1\u5ddd\u548c\u5f18\uff08\u30b7\u30c1\u30a7\u30c1\u30f3\u5927\u5b66\uff09\u300c\u539f\u59cb\u60d1\u661f\u7cfb\u5186\u76e4\u306b\u304a\u3051\u308b\u30ae\u30e3\u30c3\u30d7\u69cb\u9020\u3068\u5de8\u5927\u60d1\u661f\u300d<\/td>\n<\/tr>\n
    \u7b2c38\u56de<\/td>\n[\u7b2c28.5\u56de\u306b\u5bfe\u3059\u308b\u756a\u53f7\u8abf\u6574]<\/td>\n<\/tr>\n
    \u7b2c37\u56de<\/td>\n2016\/11\/25<\/td>\n\u6fa4\u7530\u4f50\u85e4\u8061\u5b50\uff08\u9e7f\u5150\u5cf6\u5927\u5b66\uff09\u300cAGN torus traced by molecular absorption lines\u300d<\/td>\n<\/tr>\n
    \u7b2c36\u56de<\/td>\n2016\/10\/13<\/td>\nBurns, Ross\uff08JIVE; the Netherlands\uff09\u300cRecent and future activities in maser VLBI\u300d<\/td>\n<\/tr>\n
    \u7b2c35\u56de<\/td>\n2016\/10\/ 7<\/td>\n\u5927\u6d5c\u6676\u751f\u3001\u5824\u5927\u9678\uff08\u540d\u53e4\u5c4b\u5927\u5b66\u5929\u4f53\u7269\u7406\u5b66\u7814\u7a76\u5ba4\uff09\u300c\u4e00\u9178\u5316\u70ad\u7d20\u8f1d\u7dda\u89b3\u6e2c\u306b\u3088\u308b\u661f\u9593\u7269\u8cea\u306e\u7814\u7a76\uff5eNASCO\u8a08\u753b\u306b\u5411\u3051\u3066\uff5e\u300d<\/td>\n<\/tr>\n
    \u7b2c34\u56de<\/td>\n2016\/ 9\/30<\/td>\n\u4eca\u4e95\u3000\u88d5(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300c\u591a\u6ce2\u9577\u30d0\u30f3\u30c9VLBI\u89b3\u6e2c\u5b9f\u73fe\u306b\u5411\u3051\u3066\uff1a HINOTORI\u306e\u7d39\u4ecb\u300d<\/td>\n<\/tr>\n
    \u7b2c33\u56de<\/td>\n2016\/ 7\/19<\/td>\n\u4e80\u91ce\u8aa0\u4e8c(\u56fd\u7acb\u5929\u6587\u53f0\u30c1\u30ea\u89b3\u6e2c\u6240)\u300c\u30c1\u30ea\u3068\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u300d<\/td>\n<\/tr>\n
    \u7b2c32\u56de<\/td>\n2016\/ 6\/15<\/td>\n\u9854\u58eb\u97cb[Yen Hsi-Wei] (\u53f0\u6e7e\u4e2d\u592e\u7814\u7a76\u9662\u5929\u6587\u53ca\u5929\u6587\u7269\u7406\u7814\u7a76\u6240)\u300cObservational Studies on Formation of Protoplanetary Disks\u300d<\/td>\n<\/tr>\n
    \u7b2c31\u56de<\/td>\n2016\/ 4\/16<\/td>\n\u8d64\u5800\u5353\u4e5f (\u9e7f\u5150\u5cf6\u5927\u5b66)\u300c\u643a\u5e2f\u96fb\u8a71\u306e\u5468\u6ce2\u6570\u5e2f\u3067\u63a2\u308b\u5b87\u5b99\u306e\u78c1\u5316\u30d7\u30e9\u30ba\u30de\u300d<\/td>\n<\/tr>\n
    \u7b2c30\u56de<\/td>\n2016\/ 4\/ 5<\/td>\nWillem Baan(ASTRON\u540d\u8a89\u6559\u6388\uff09\u300cInterpreting Molecules and Masers[\u661f\u9593\u5206\u5b50\u53ca\u3073\u30e1\u30fc\u30b6\u30fc\u306e\u89e3\u91c8\u306b\u3064\u3044\u3066]\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2015\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n
    \u7b2c29\u56de<\/td>\n2016\/ 2\/26<\/td>\nJames Chibueze (University of Nigeria)\u300cMulti-wavelength View of High-mass Star formation: Future AVN Contribution\u300d<\/td>\n<\/tr>\n
    \u7b2c28.5\u56de<\/td>\n2016\/ 2\/16<\/td>\nDr. Richard Paul Armstrong (\u30b1\u30fc\u30d7\u30bf\u30a6\u30f3\u5927\u5b66)\u300cFast Radio Transients with MeerKAT\u300d<\/td>\n<\/tr>\n
    \u7b2c28\u56de<\/td>\n2016\/ 1\/19<\/td>\n\u9ad8\u6851\u7e41\u4e45\uff08ASIAA\u53f0\u6e7e\u4e2d\u592e\u7814\u7a76\u9662\u5929\u6587\u53ca\u5929\u6587\u7269\u7406\u7814\u7a76\u6240\uff09\u300cSMA\u3068ALMA\u306b\u3088\u308b\u539f\u59cb\u661f\u9023\u661f\u306e\u89b3\u6e2c\u7684\u7814\u7a76\u300d<\/td>\n<\/tr>\n
    \u7b2c27\u56de<\/td>\n2015\/10\/ 8<\/td>\nSteve Goldman\uff08Keele University\uff09\u300cThe evolution and mass loss of AGB and RSG stars\u300d<\/td>\n<\/tr>\n
    \u7b2c26\u56de<\/td>\n2015\/ 8\/ 7<\/td>\n\u53e4\u5c4b\u3000\u73b2\uff08\u5fb3\u5cf6\u5927\u5b66\uff09\u300c\u4e71\u6d41\u3068\u78c1\u5834\u3067\u652f\u3048\u3089\u308c\u305f\u30d5\u30a3\u30e9\u30e1\u30f3\u30c8\u72b6\u5206\u5b50\u96f2\u3067\u5f62\u6210\u3055\u308c\u305f\u66b4\u8d70\u7684\u306b\u53ce\u7e2e\u3059\u308b\u5206\u5b50\u96f2\u30b3\u30a2\u304a\u3088\u3073\u300e\u539f\u59cb\u7684\u5206\u5b50\u96f2\u30b3\u30a2\u300f\u306e\u767a\u898b\u300d<\/td>\n<\/tr>\n
    \u7b2c25\u56de<\/td>\n2015\/ 7\/24<\/td>\n\u8868 \u5be6\uff08\u6176\u61c9\u7fa9\u587e\u5927\u5b66\uff09\u300c\u30a4\u30f3\u30bf\u30fc\u30cd\u30c3\u30c8\u671b\u9060\u93e1\u30cd\u30c3\u30c8\u30ef\u30fc\u30af\u304c\u5207\u308a\u958b\u304f\u5929\u6587\u5b66\u6559\u80b2\u306e\u65b0\u305f\u306a\u53ef\u80fd\u6027\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2014\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c24\u56de<\/td>\n2015\/ 3\/6<\/td>\n\u7530\u6751\u9686\u5e78\uff08JAXA \u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240\uff09\u300cX\u7dda\u3067\u63a2\u308b\u5b87\u5b99\u306e\u5927\u898f\u6a21\u69cb\u9020\u3068\u6697\u9ed2\u7269\u8cea\u300d\uff08\u8b1b\u5e2b\u4f53\u8abf\u4e0d\u826f\u306e\u305f\u3081\u53d6\u6d88\uff09<\/del><\/td>\n<\/tr>\n
    \u7b2c23\u56de<\/td>\n2015\/ 1\/14<\/td>\n\u9577\u5c3e\u900f(\u611b\u5a9b\u5927\u5b66)\u300cSubaru Wide-Field AGN Survey (SWANS) with HSC\u300d<\/td>\n<\/tr>\n
    \u7b2c22\u56de<\/td>\n2014\/12\/4<\/td>\n\u5409\u4e95\u8b93(\u6771\u4eac\u5927\u5b66)\u300c\u6771\u4eac\u5927\u5b66\u30a2\u30bf\u30ab\u30de\u5929\u6587\u53f0(TAO)\u30d7\u30ed\u30b8\u30a7\u30af\u30c8\u300d<\/td>\n<\/tr>\n
    \u7b2c21\u56de<\/td>\n2014\/11\/10<\/td>\nRyan Shannon (CSIRO Astronomy and Space Science)\u300cConstraining the Supermassive Black Hole Population with Gravitational Waves and Pulsar Timing Arrays\u300d<\/td>\n<\/tr>\n
    \u7b2c16\u56de<\/td>\n2014\/ 9\/29<\/td>\nRoss Burns(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300ctrigonometric distance to IRAS20056+3350: massive star forming region on the solar circle\u300d<\/td>\n<\/tr>\n
    \u7b2c20\u56de<\/td>\n2014\/ 9\/19<\/td>\nGabor Oroz(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300cEvolutionary diagnostics of AGB stars using time variation of maser species\u300d<\/td>\n<\/tr>\n
    \u7b2c19\u56de<\/td>\n2014\/ 7\/25<\/td>\nGabor Oroz(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300cExploration of high precision astrometry for stellar maser sources with very long baseline interferometry\u300d<\/td>\n<\/tr>\n
    \u7b2c18\u56de<\/td>\n2014\/ 7\/16<\/td>\nRoss Burns(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300cUsing archival infra-red data as diagnostics for star forming regions\u300d<\/td>\n<\/tr>\n
    \u7b2c17\u56de<\/td>\n2014\/ 7\/14<\/td>\n\u4e80\ufa11\u9054\u4e5f(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300cNGC2264C\u9818\u57df\u306e\u8ddd\u96e2\u6e2c\u5b9a\u3068\uff38\u7dda\u653e\u5c04\u3092\u4f34\u3046\u30af\u30e9\u30b9\uff10\u5019\u88dc\u5929\u4f53\u300d<\/td>\n<\/tr>\n
    \u7b2c16\u56de<\/td>\n2014\/ 7\/10<\/td>\n(\u66b4\u98a8\u96e8\u306b\u3088\u308b\u5927\u5b66\u9589\u9396\u306e\u305f\u30812014\/9\/29\u306b\u5ef6\u671f)<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2013\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n\n\n\n\n\n
    \u7b2c15\u56de<\/td>\n2014\/ 1\/17<\/td>\n\u4e8c\u9593\u702c\u654f\u53f2(\u6771\u5317\u5927\u5b66)\u300c\u5f31\u3044\u91cd\u529b\u30ec\u30f3\u30ba\u306b\u3088\u308b\u5b87\u5b99\u306e\u69cb\u9020\u5f62\u6210\u7406\u8ad6\u306e\u691c\u8a3c\u300d<\/td>\n<\/tr>\n
    \u7b2c14\u56de<\/td>\n2014\/ 1\/10<\/td>\nRoss Burns(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300cThe role of disks in high mass star formation\u300d<\/td>\n<\/tr>\n
    \u7b2c13\u56de<\/td>\n2013\/12\/ 6<\/td>\n\u4e80\ufa11\u9054\u77e2(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300c\u661f\u5f62\u6210\u9818\u57dfNGC2264C\u3068X\u7dda\u6e90\u300d<\/td>\n<\/tr>\n
    \u7b2c12\u56de<\/td>\n2013\/11\/b5<\/td>\n\u798f\u4e95\u5eb7\u96c4(\u540d\u53e4\u5c4b\u5927\u5b66)\u300cA new tool to measure dense HI gas based on the Planck dust properties: Evidence for massive HI envelopes surrounding CO clouds\u300d<\/td>\n<\/tr>\n
    \u7b2c11\u56de<\/td>\n2013\/10\/11<\/td>\n\u5c0f\u6797\u79c0\u884c(\u56fd\u7acb\u5929\u6587\u53f0)\u300c\u56fd\u7acb\u5929\u6587\u53f0\u306e\u4eca\u5f8c10\u5e74\u9593\u300d<\/td>\n<\/tr>\n
    \u7b2c10\u56de<\/td>\n2013\/b8\/ b9<\/td>\n\u4e80\ufa11\u9054\u77e2(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300c\u661f\u5f62\u6210\u9818\u57dfNGC2264\u3068X\u7dda\u6e90\u300d<\/td>\n<\/tr>\n
    \u7b2c\uff19\u56de<\/td>\n2013\/ 7\/19<\/td>\nRoss Burns (Kagoshima University)\u300cStructure and Kinematics of the Milky Way based VERA observations of IRAS 20143+3634, IRAS 20056+3350 and other maser sources\u300d<\/td>\n<\/tr>\n
    \u7b2c\uff18\u56de<\/td>\n2013\/ 4\/26<\/td>\nOrosz Gabor (Budapest University of Technology)\u300cOptical\u2013radio positional offsets for active galactic nuclei\u300d<\/td>\n<\/tr>\n
    \u7b2c\uff17\u56de<\/td>\n2013\/ 4\/18<\/td>\n\u4eca\u4e95\u3000\u88d5(\u9e7f\u5150\u5cf6\u5927\u5b66)\u300c\u897f\u30aa\u30fc\u30b9\u30c8\u30e9\u30ea\u30a2\u6ede\u5728\u5831\u544a\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2012\u5e74\u5ea6<\/h4>\n\n\n\n\n\n\n
    \u7b2c\uff16\u56de<\/td>\n2013\/ 2\/28<\/td>\n\u7802\u7530\u548c\u826f(\u56fd\u7acb\u5929\u6587\u53f0)\u300cFar-infrared properties of YSOs\u300d<\/td>\n<\/tr>\n
    \u7b2c\uff15\u56de<\/td>\n2012\/12\/ 5<\/td>\n\u90f7\u7530\u76f4\u8f1d(\u56fd\u7acb\u5929\u6587\u53f0)\u300c\u8d64\u5916\u7dda\u4f4d\u7f6e\u5929\u6587\u89b3\u6e2c\u885b\u661fJASMINE\u8a08\u753b\u3068\u9280\u6cb3\u7cfb\u63a2\u6c42\u300d<\/td>\n<\/tr>\n
    \u7b2c\uff14\u56de<\/td>\n2012\/ 7\/17<\/td>\nMatin Bureau(Oxford University)\u300cObserving Galaxies in 3D\u300d<\/td>\n<\/tr>\n
    \u7b2c\uff13\u56de<\/td>\n2012\/ 4\/13<\/td>\nRoss Burns(Cardiff University\/\u9e7f\u5150\u5cf6\u5927\u5b66)<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

    2011\u5e74\u5ea6<\/h4>\n\n\n\n\n
    \u7b2c\uff12\u56de<\/td>\n2012\/ 2\/07<\/td>\n\u6797\u6b63\u5f66(\u56fd\u7acb\u5929\u6587\u53f0)<\/td>\n<\/tr>\n
    \u7b2c\uff11\u56de<\/td>\n2012\/ 1\/17<\/td>\n\u677e\u6c38\u5178\u4e4b(\u6771\u4eac\u5927\u5b66)\u300c\u9280\u6cb3\u7cfb\u4e2d\u5fc3\u9818\u57df\u306e\u5909\u5149\u661f\u63a2\u67fb\u300d<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n

    <\/p>\n","protected":false},"excerpt":{"rendered":"

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[…]<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_acf_changed":false,"_locale":"ja","_original_post":"http:\/\/agarc.sci.kagoshima-u.ac.jp\/wordpress\/?page_id=55","footnotes":""},"class_list":["post-55","page","type-page","status-publish","hentry","ja"],"acf":[],"yoast_head":"\n\u9e7f\u5150\u5cf6\u5927\u5b66\u5929\u6587\u5b66\u8ac7\u8a71\u4f1a | \u5929\u306e\u5ddd\u9280\u6cb3\u7814\u7a76\u30bb\u30f3\u30bf\u30fc\u3000\u9e7f\u5150\u5cf6\u5927\u5b66\u5927\u5b66\u9662\u3000\u7406\u5de5\u5b66\u7814\u7a76\u79d1\u9644\u5c5e<\/title>\n<meta name=\"description\" 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