{"id":1963,"date":"2023-11-08T09:55:12","date_gmt":"2023-11-08T00:55:12","guid":{"rendered":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/?p=1963"},"modified":"2023-11-08T09:55:12","modified_gmt":"2023-11-08T00:55:12","slug":"2023-11-22","status":"publish","type":"post","link":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/2023\/11\/08\/2023-11-22\/","title":{"rendered":"2023-11-22"},"content":{"rendered":"\n<h2 class=\"wp-block-heading has-bright-blue-color has-text-color\">The distribution of magnetic field strengths in star-forming regions<\/h2>\n\n\n\n<p class=\"has-text-align-right\">Speaker: Jihye Hwang<\/p>\n\n\n\n<p>Abstract:<\/p>\n\n\n\n<p> \u201cWhat is the role of magnetic fields for regulating star-forming processes?\u201d It is a long- standing issue in star formation studies. To judge the exact role of magnetic fields in star-forming regions, it is necessary to estimate the magnetic field strengths of those regions. However, previous studies have estimated a mean magnetic field strength in a whole star-forming region. I suggest a new application to estimate the distribution of magnetic field strengths in a star-forming region. I applied this towards three star-forming regions, the OMC-1 region, Mon R2 and G28.34 using POL-2\/SCUBA-2 on the James Clerk Maxwell Telescope. In this talk, I will show the magnetic field strengths in those regions and discuss the relative importance between magnetic field, turbulence and gravity.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The distribution of magnetic field strengths in star-forming regions Speaker: Jihye Hwang Abstract: \u201cWhat is t &hellip; <a href=\"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/2023\/11\/08\/2023-11-22\/\" class=\"more-link\"><span class=\"screen-reader-text\">&#8220;2023-11-22&#8221; \u306e<\/span>\u7d9a\u304d\u3092\u8aad\u3080<\/a><\/p>\n","protected":false},"author":27,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-1963","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\/1963","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\/27"}],"replies":[{"embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/comments?post=1963"}],"version-history":[{"count":1,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/1963\/revisions"}],"predecessor-version":[{"id":1964,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/1963\/revisions\/1964"}],"wp:attachment":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/media?parent=1963"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/categories?post=1963"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/tags?post=1963"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}