{"id":9688,"date":"2018-08-21T10:30:20","date_gmt":"2018-08-21T07:30:20","guid":{"rendered":"http:\/\/www.inasan.ru\/?p=9688"},"modified":"2018-08-21T10:30:20","modified_gmt":"2018-08-21T07:30:20","slug":"seminar_0385","status":"publish","type":"post","link":"http:\/\/www.inasan.ru\/en\/seminar_0385\/","title":{"rendered":"Astrophysical Seminar (27 August  2018, 11:00)"},"content":{"rendered":"<p><b>1) Speaker:<\/b> <em>D. Ojha (Tata Institute of Fundamental Research, Mumbai, India)<br \/>\n<\/em><\/p>\n<p><b>Title:<\/b>\u00a0 &#8220;<em>Observational Aspects of Triggered Star Formation in the Milky Way&#8221;<\/em><\/p>\n<p><b>Abstract: <br \/>\n<\/b><\/p>\n<p>Since last few years we are pursuing multiwavelength (optical, infrared, sub-mm, mm and radio) studies of Galactic star-forming regions. The use of multiwavelength data is essential to investigate the ionized, neutral, and molecular components of the gas, the dust, and the population of young stellar objects. A variety of Galactic H II regions (bright, faint, smaller, nearby and distant) have been explored. Evidence of direct interactions between the H II regions, molecular gas and the young stellar objects has been found on large and small scales. In this talk, I will present the recent results from our ongoing investigation of triggered star formation at the periphery Galactic H II regions.<\/p>\n<p>In the second part of my talk, I will give a brief description of the activities of the Infrared Astronomy Group (Department of Astronomy &amp; Astrophysics) of TIFR with special emphasis on space-based far-infrared (balloon-borne) and ground-based near-infrared Instrumentation for star formation studies.<\/p>\n<p><strong><a href=\"http:\/\/www.inasan.ru\/en\/scientific_activities\/seminars\/inasan_astrophysical_seminar\/\">Sign up for the seminar<\/a><\/strong><\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>1) Speaker: D. Ojha (Tata Institute of Fundamental Research, Mumbai, India) Title:\u00a0 &#8220;Observational Aspects of Triggered Star Formation in the Milky Way&#8221; Abstract: Since last few years we are pursuing multiwavelength (optical, infrared, sub-mm, mm and radio) studies of Galactic star-forming regions. The use of multiwavelength data is essential to investigate the ionized, neutral, and<\/p>\n<div class=\"read-more\"><a href=\"http:\/\/www.inasan.ru\/en\/seminar_0385\/\">Continue Reading&rsaquo;&rsaquo;<\/a><\/div>\n","protected":false},"author":12,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6],"tags":[],"class_list":["post-9688","post","type-post","status-publish","format-standard","hentry","category-seminar"],"translation":{"provider":"WPGlobus","version":"3.0.0","language":"en","enabled_languages":["ru","en"],"languages":{"ru":{"title":true,"content":true,"excerpt":false},"en":{"title":true,"content":true,"excerpt":false}}},"_links":{"self":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/9688","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/users\/12"}],"replies":[{"embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/comments?post=9688"}],"version-history":[{"count":3,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/9688\/revisions"}],"predecessor-version":[{"id":9701,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/9688\/revisions\/9701"}],"wp:attachment":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/media?parent=9688"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/categories?post=9688"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/tags?post=9688"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}