{"id":80,"date":"2010-10-15T15:10:46","date_gmt":"2010-10-15T06:10:46","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog2\/?p=80"},"modified":"2010-10-15T15:10:46","modified_gmt":"2010-10-15T06:10:46","slug":"scattered_radiation_field_and","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=80","title":{"rendered":"Scattered Radiation Field and Local Magnetic Field of the Protostellar Clusters in NGC 2264"},"content":{"rendered":"<p>\u3010\u65e5\u6642\u301110\u670813\u65e5(\u6c34)\u300010:30\uff5e12:00<br \/>\n\u3010\u5834\u6240\u3011\u56fd\u7acb\u5929\u6587\u53f0\u30fb\u4e09\u9df9\u3000\u4e2d\u592e\u68df\uff08\u5317\uff091\u968e \u8b1b\u7fa9\u5ba4<br \/>\n\u3010\u767a\u8868\u8005\uff08\u656c\u79f0\u7565\uff09\u3011Kwon Jungmi\uff08\u7dcf\u7814\u5927 D1\u30fb\u4e09\u9df9\u3001\u6307\u5c0e\u6559\u54e1 : \u7530\u6751 \u5143\u79c0\uff09<br \/>\n\u3010\u30bf\u30a4\u30c8\u30eb\u3011Scattered Radiation Field and Local Magnetic Field of the Protostellar Clusters in NGC 2264<br \/>\nThe NGC 2264 IRS 2 region in the Mon OB 1 cloud was observed in the near-infrared (IR) J, H, and Ks bands, and imaging polarimetry was performed.<br \/>\nOur polarization data revealed various infrared reflection nebulae (IRNe) associated with the central IR young star cluster NGC 2264 IRAS 12 S1 core and identified their illuminating sources, and revealed at least three infrared reflection nebula cluster (IRNCs).<br \/>\nIn addition, 270 point-like sources w ere detected in all three bands.<br \/>\nThe near-IR polarizations of these sources seem to be caused mostly by the dichroic extinction.<br \/>\nThe mean polarization position angle of sources with P \/\u03b4P 3 is about 68\u00b0, which is interpreted as the projected direction of the magnetic field in the observed region of the cloud.<br \/>\nThe distribution of the polarization angle has a dispersion of about 27\u00b0.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>\u3010\u65e5\u6642\u301110\u670813\u65e5(\u6c34)\u300010:30\uff5e12:00 \u3010\u5834\u6240\u3011\u56fd\u7acb\u5929\u6587\u53f0\u30fb\u4e09\u9df9\u3000\u4e2d\u592e\u68df\uff08\u5317\uff091\u968e \u8b1b\u7fa9\u5ba4 \u3010\u767a\u8868\u8005\uff08\u656c\u79f0\u7565\uff09\u3011Kwon Jungmi\uff08\u7dcf\u7814\u5927 D1\u30fb\u4e09\u9df9\u3001\u6307\u5c0e\u6559\u54e1 : \u7530\u6751 \u5143\u79c0\uff09 \u3010\u30bf\u30a4\u30c8\u30eb\u3011Scatte [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,5],"tags":[],"class_list":["post-80","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\/80","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=80"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/80\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=80"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=80"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=80"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}