{"id":752,"date":"2017-06-14T13:34:00","date_gmt":"2017-06-14T04:34:00","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=752"},"modified":"2017-06-15T09:36:07","modified_gmt":"2017-06-15T00:36:07","slug":"3d-radiation-mhd-simulation-of-clumpy-outflow-from-supercritical-accretion-flow-understanding-the-dynamics-of-jetoutflow-driven-by-high-mass-young-stellar-objects-based-on-22-ghz-water-maser-survey","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=752","title":{"rendered":"3D Radiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow \/ Understanding the dynamics of jet\/outflow driven by high-mass young stellar objects based on 22 GHz water maser survey using KaVA."},"content":{"rendered":"<p>[Speaker1]<br \/>\nHiroshi Kobayashi, SOKENDAI (Supervisor; Ken Ohsuga)<br \/>\n[Title]<br \/>\n3D Radiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow<\/p>\n<p>[Speaker2]<br \/>\nJungha Kim, SOKENDAI (Supervisor; Mareki Honma, Tomoya Hirota, Katsunori Shibata)<br \/>\n[Title]<br \/>\nUnderstanding the dynamics of jet\/outflow driven by high-mass young stellar objects based on 22 GHz water maser survey using KaVA.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Hiroshi Kobayashi, SOKENDAI (Supervisor; Ken Ohsuga) [Title] 3D Radiation-MHD Simulation of Clumpy  [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,5],"tags":[],"class_list":["post-752","post","type-post","status-publish","format-standard","hentry","category-6","category-5"],"_links":{"self":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/752","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=752"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/752\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=752"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=752"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=752"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}