{"id":1676,"date":"2021-12-15T14:33:30","date_gmt":"2021-12-15T05:33:30","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1676"},"modified":"2022-01-12T14:46:54","modified_gmt":"2022-01-12T05:46:54","slug":"study-on-the-debris-disk-of-an-m-type-star-au-mic-by-fast-pdi-mode-of-subaru-telescope-a-new-measurement-method-of-isotopologue-ratios-in-protoplanetary-disks-a-case-study-of-the-12co-13co-ratio","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1676","title":{"rendered":"Study on the Debris Disk of an M-type star, AU Mic, by Fast PDI mode of Subaru Telescope \/  A new measurement method of isotopologue ratios in protoplanetary disks: a case study of the 12CO\/13CO ratio in the TW Hya disk"},"content":{"rendered":"<p>[Speaker1]<br \/>\nShiori Koshisaka<br \/>\nSOKENDAI 1st year (M1)<br \/>\n(Supervisor: Takayuki Kotani, Misato Fukagawa, Yasunori Hori)<br \/>\n[Title1]<br \/>\nStudy on the Debris Disk of an M-type star, AU Mic, by Fast PDI mode of Subaru Telescope<\/p>\n<p>[Speaker2]<br \/>\nTomohiro Yoshida<br \/>\nSOKENDAI 1st year (M1)<br \/>\n(Supervisor: Hideko Nomura, Misato Fukagawa, Akimasa Kataoka)<br \/>\n[Title2]<br \/>\nA new measurement method of isotopologue ratios in protoplanetary disks: a case study of the 12CO\/13CO ratio in the TW Hya disk<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Shiori Koshisaka SOKENDAI 1st year (M1) (Supervisor: Takayuki Kotani, Misato Fukagawa, Yasunori Hor [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,2],"tags":[],"class_list":["post-1676","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\/1676","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=1676"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1676\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1676"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1676"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1676"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}