{"id":4766,"date":"2016-06-24T12:34:19","date_gmt":"2016-06-24T09:34:19","guid":{"rendered":"http:\/\/www.inasan.ru\/?p=4766"},"modified":"2016-06-24T12:52:46","modified_gmt":"2016-06-24T09:52:46","slug":"seminar_0327","status":"publish","type":"post","link":"http:\/\/www.inasan.ru\/en\/seminar_0327\/","title":{"rendered":"Astrophysical Seminar (30 June 2016, 11:00)"},"content":{"rendered":"<p><b>Speaker:<\/b> <i><span style=\"color: #0000ff;\">L.I. Mashonkina (INASAN)<\/span><\/i><\/p>\n<p><b>Title:<\/b> <i><span style=\"color: #0000ff;\">&#8220;Detailed chemical abundances of Li to Eu in the F-G dwarfs of different metallicity as the observational constraints to the Galactic chemical evolution models&#8221;<\/span><\/i><\/p>\n<p><b>Abstract:<\/b><\/p>\n<p>We present results of the 5-year long work of a large team of collaborators from the four countries on the determination of atmospheric parameters and chemical abundances of Li to Eu for the F-G dwarf sample covering the metallicity range -2.7 < [Fe\/H] < 0.3. The results are based on analysis of high-resolution spectral observations and the non-LTE line formation. The obtained elemental ratios are compared with the modern models of the Galactic chemical evolution.\n\n\n\n<p><span style=\"color: #000080;\"><strong><a style=\"color: #000080;\" href=\"http:\/\/www.inasan.ru\/scientific_activities\/seminars\/inasan_astrophysical_seminar\/\">Sign up for the seminar<\/a><\/strong><\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Speaker: L.I. Mashonkina (INASAN) Title: &#8220;Detailed chemical abundances of Li to Eu in the F-G dwarfs of different metallicity as the observational constraints to the Galactic chemical evolution models&#8221; Abstract: We present results of the 5-year long work of a large team of collaborators from the four countries on the determination of atmospheric parameters and<\/p>\n<div class=\"read-more\"><a href=\"http:\/\/www.inasan.ru\/en\/seminar_0327\/\">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-4766","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\/4766","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=4766"}],"version-history":[{"count":10,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/4766\/revisions"}],"predecessor-version":[{"id":4768,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/4766\/revisions\/4768"}],"wp:attachment":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/media?parent=4766"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/categories?post=4766"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/tags?post=4766"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}