{"id":2056,"date":"2023-07-19T12:00:44","date_gmt":"2023-07-19T03:00:44","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=2056"},"modified":"2023-07-18T13:06:39","modified_gmt":"2023-07-18T04:06:39","slug":"the-history-of-mass-ratio-determination-of-x-ray-binary-ss433-observational-study-of-the-fragmentation-process-in-nearby-star-forming-regions","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=2056","title":{"rendered":"SOKENDAI Colloquium (2023.7.19)"},"content":{"rendered":"<p>Speaker1 : Miho Tan<br \/>\nAffiliation: SOKENDAI 1st year (M1)<br \/>\n(Supervisor: Mami Machida, Tomoya Takiwaki, Kazunari Iwasaki)<br \/>\nTitle: The history of mass ratio determination of X-Ray Binary SS433<\/p>\n<p>Speaker2 : Kousuke Ishihara<br \/>\nAffiliation: SOKENDAI 4th year (D2)<br \/>\n(Supervisor: Masao Saito, Fumitaka Nakamura, Patricio Sanhueza)<br \/>\nTitle: Observational study of the fragmentation process in nearby star-forming regions<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Speaker1 : Miho Tan Affiliation: SOKENDAI 1st year (M1) (Supervisor: Mami Machida, Tomoya Takiwaki, Kazunari I [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,2],"tags":[],"class_list":["post-2056","post","type-post","status-publish","format-standard","hentry","category-6","category-2"],"_links":{"self":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/2056","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=2056"}],"version-history":[{"count":3,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/2056\/revisions"}],"predecessor-version":[{"id":2059,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/2056\/revisions\/2059"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=2056"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=2056"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=2056"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}