[Speaker 1]
\nOh Daehyeon D2, SOKENDAI, Mitaka\uff08supervisor : Woko Aoki\uff09
\n[Title]
\nThe widest separation and low mass planetarymass companion(PMC) candidates around DoAr 25
\n[Abstract]
\n–<\/p>\n
[Speaker 2]
\nYang Yi M2, SOKENDAI, Mitaka\uff08supervisor : Saeko Hayashi\uff09
\n[Title]
\nDirect Imaging of DM Tau in NIR Band
\n[Abstract]
\nCircumstellar disks are often observed to be surrounding young stars, especially T Tauri stars. The composition and structure of circumstellar disks have essential effect in the formation of planets. Therefore, investigation of such disks is quite beneficial for us to understand the formation process of the planetary system. In this presentation, I will show the near infrared observation of DM Tau from HiCIAO instrument mounted on Subaru Telescope. This T Tauri star is located in Taurus star formation region which is one of the nearest star formation regions from the Solar System. Hence it is easy to resolve the detailed structure of its disk. I believe this research is quite helpful to figure out the scenario of disk evolution and the ongoing planet formation in that disk. <\/p>\n","protected":false},"excerpt":{"rendered":"
[Speaker 1] Oh Daehyeon D2, SOKENDAI, Mitaka\uff08supervisor : Woko Aoki\uff09 [Title] The widest separation and low mas […]<\/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-192","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\/192","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=192"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/192\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=192"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=192"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=192"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}