{"id":1375,"date":"2022-01-26T09:06:37","date_gmt":"2022-01-26T00:06:37","guid":{"rendered":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/?p=1375"},"modified":"2022-01-26T09:06:37","modified_gmt":"2022-01-26T00:06:37","slug":"2022-02-02","status":"publish","type":"post","link":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/2022\/01\/26\/2022-02-02\/","title":{"rendered":"2022-02-02"},"content":{"rendered":"\n<p class=\"has-bright-blue-color has-text-color\" style=\"font-size:24px\">Towards more detailed modeling of galaxy formation<\/p>\n\n\n\n<p class=\"has-text-align-right\">Speaker: Takashi Okamoto<\/p>\n\n\n\n<p>Abstract:\u00a0<\/p>\n\n\n\n<p>Current cosmological simulations of galaxy formation have been successful&nbsp;in explaining many observed properties of galaxies. There are, however, some&nbsp;tensions between the simulations and observations. I briefly describe the&nbsp;current status of simulations of galaxy formation. I then introduce our recent attempts&nbsp;to develop new star formation recipes in galaxy scale simulations. The new method allows&nbsp;us to identify star-forming clouds and detect collisions between the clouds during&nbsp;galaxy-scale simulations. I show some preliminary results obtained by a collision-induced&nbsp;star formation model.&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Towards more detailed modeling of galaxy formation Speaker: Takashi Okamoto Abstract:\u00a0 Current cosmological si &hellip; <a href=\"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/2022\/01\/26\/2022-02-02\/\" class=\"more-link\"><span class=\"screen-reader-text\">&#8220;2022-02-02&#8221; \u306e<\/span>\u7d9a\u304d\u3092\u8aad\u3080<\/a><\/p>\n","protected":false},"author":17,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-1375","post","type-post","status-publish","format-standard","hentry","category-1"],"_links":{"self":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/1375","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/users\/17"}],"replies":[{"embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/comments?post=1375"}],"version-history":[{"count":1,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/1375\/revisions"}],"predecessor-version":[{"id":1376,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/1375\/revisions\/1376"}],"wp:attachment":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/media?parent=1375"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/categories?post=1375"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/tags?post=1375"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}