{"id":461,"date":"2015-06-25T10:43:28","date_gmt":"2015-06-25T01:43:28","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=461"},"modified":"2016-06-16T11:33:36","modified_gmt":"2016-06-16T02:33:36","slug":"supermassive-black-hole-mass-estimation-using-molecular-gas-kinematics-observed-with-millimetersubmillimeter-interferometor","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=461","title":{"rendered":"Supermassive Black Hole Mass Estimation Using Molecular Gas Kinematics Observed with Millimeter\/Submillimeter Interferometor"},"content":{"rendered":"<p>[Speaker1]<br \/>\nKyoko Onishi, D2, SOKENDAI, Mitaka(supervisor: Satoru Iguchi)<br \/>\n[Title]<br \/>\nSupermassive Black Hole Mass Estimation Using Molecular Gas Kinematics Observed with Millimeter\/Submillimeter Interferometor<br \/>\n[Abstract]<br \/>\nUbiquitely present at the centres of galaxies, supermassive black holes (SMBHs) are key to understand galaxy evolution. However, the SMBH mass-central velocity dispersion relation, which is driving most theoretical efforts, is based on a relatively small number of measurements and only a handful of methods.<br \/>\nOur recent work has shown that it is straightforward to dynamically estimate the mass of SMBHs, by simply probing the near-Keplerian rotation of molecular disks around them at high angular resolution. In the ALMA era, this can yield hundreds of measurements in galaxies of all morphological types.<br \/>\nIn the talk, I will show the SMBH mass measurement in NGC 1097 by using ALMA Cycle 0 observation, and also in NGC 3665 by using CARMA observation.<\/p>\n<p>[Speaker2]<br \/>\nKoki Okutomi, D1, SOKENDAI, Mitaka(supervisor: Yoichi Aso)<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Kyoko Onishi, D2, SOKENDAI, Mitaka(supervisor: Satoru Iguchi) [Title] Supermassive Black Hole Mass  [&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-461","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\/461","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=461"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/461\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=461"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=461"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=461"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}