{"id":625,"date":"2016-06-29T15:44:57","date_gmt":"2016-06-29T06:44:57","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=625"},"modified":"2016-06-29T15:44:57","modified_gmt":"2016-06-29T06:44:57","slug":"multi-color-simultaneous-observations-of-the-transiting-hot-jupiter-candidate-13c-isotopic-fractionation-of-hc3n-in-star-forming-regions","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=625","title":{"rendered":"Multi-color simultaneous observations of the transiting hot Jupiter candidate \/ 13C isotopic fractionation of HC3N in star forming regions"},"content":{"rendered":"<p>[Speaker 1]<br \/>\nShogo Ishikawa, D3, SOKENDAI (Supervisor: Nobunari Kashikawa)<\/p>\n<p>[Speaker 2]\u3000<br \/>\nMasahiro Onitsuka, D3, SOKENDAI(supervisor: Tomonori Usuda)<br \/>\n[Title]<br \/>\nMulti-color simultaneous observations of the transiting hot Jupiter candidate<\/p>\n<p>[Speaker3]<br \/>\nKotomi Taniguchi, D2, SOKENDAI (Supervisor; Masao Saito)<br \/>\n[Title]<br \/>\n13C isotopic fractionation of HC3N in star forming regions<br \/>\n[Abstract]<br \/>\nI will talk about observations with the Nobeyama 45-m telescope during this observational season. We investigate 13C isotopic fractionation of HC3N and discuss its main formation mechanisms in L1527 and G28.28-0.36.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker 1] Shogo Ishikawa, D3, SOKENDAI (Supervisor: Nobunari Kashikawa) [Speaker 2]\u3000 Masahiro Onitsuka, D3,  [&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-625","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\/625","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=625"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/625\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=625"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=625"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=625"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}