{"id":700,"date":"2017-01-25T15:34:01","date_gmt":"2017-01-25T06:34:01","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=700"},"modified":"2017-01-26T15:38:57","modified_gmt":"2017-01-26T06:38:57","slug":"analysis-of-molecular-lines-in-the-near-infrared-high-dispersion-spectra-of-barnards-star-understanding-the-circumstellar-structure-of-high-mass-young-stellar-objects-based-on-kava-observat","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=700","title":{"rendered":"Analysis of Molecular Lines in the Near-Infrared High Dispersion Spectra of Barnard\u2019s Star \/ Understanding the circumstellar structure of high-mass young stellar objects based on KaVA observations"},"content":{"rendered":"<p>[Speaker1]<br \/>\nHiroyuki Ishikawa, M1, SOKENDAI (Supervisor; Takayuki Kotani)<br \/>\n[Title]<br \/>\nAnalysis of Molecular Lines in the Near-Infrared High Dispersion Spectra of Barnard\u2019s Star<\/p>\n<p>[Speaker2]<br \/>\nJungha Kim, D1, SOKENDAI (Supervisor; Honma Mareki)<br \/>\n[Title]<br \/>\nUnderstanding the circumstellar structure of high-mass young stellar objects based on KaVA observations <\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Hiroyuki Ishikawa, M1, SOKENDAI (Supervisor; Takayuki Kotani) [Title] Analysis of Molecular Lines i [&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-700","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\/700","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=700"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/700\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=700"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=700"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=700"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}