{"id":1753,"date":"2022-05-25T13:20:36","date_gmt":"2022-05-25T04:20:36","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1753"},"modified":"2022-05-25T13:20:36","modified_gmt":"2022-05-25T04:20:36","slug":"the-role-of-filament-filament-collision-in-star-formation-clarification-of-magnetic-field-structure-in-spiral-galaxies-by-low-frequency-simulated-polarization-observations","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1753","title":{"rendered":"The Role of Filament-Filament Collision in Star Formation \/ Clarification of Magnetic Field Structure in Spiral Galaxies by Low-Frequency Simulated Polarization Observations"},"content":{"rendered":"<p>[Speaker1]<br \/>\nRaiga Kashiwagi<br \/>\nSOKENDAI 4th year (D2)<br \/>\n(Supervisor: Kazunari Iwasaki, Tomoya Takiwaki, Nanase Harada)<br \/>\n[Title1]<br \/>\nThe Role of Filament-Filament Collision in Star Formation<\/p>\n<p>[Speaker2]<br \/>\nYuta Tashima<br \/>\nSOKENDAI 4th year (D2)<br \/>\n(Supervisor: Mami Machida, Fumitaka Nakamura, Tomoya Takiwaki)<br \/>\n[Title2]<br \/>\nClarification of Magnetic Field Structure in Spiral Galaxies by Low-Frequency Simulated Polarization Observations<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Raiga Kashiwagi SOKENDAI 4th year (D2) (Supervisor: Kazunari Iwasaki, Tomoya Takiwaki, Nanase Harad [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,2],"tags":[],"class_list":["post-1753","post","type-post","status-publish","format-standard","hentry","category-6","category-2"],"_links":{"self":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1753","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=1753"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1753\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1753"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1753"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1753"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}