\u041d\u0410\u0423\u0427\u0415\u041d \u0421\u0415\u041c\u0418\u041d\u0410\u0420<\/p>\n
\u0420\u0435\u0434\u043e\u0432\u043d\u0430\u0442\u0430 \u0441\u0431\u0438\u0440\u043a\u0430 \u043d\u0430 \u0441\u0435\u043c\u0438\u043d\u0430\u0440\u0430 \u043d\u0430 \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442\u0430 \u043f\u043e \u0410\u0441\u0442\u0440\u043e\u043d\u043e\u043c\u0438\u044f \u0449\u0435 \u0441\u0435 \u043f\u0440\u043e\u0432\u0435\u0434\u0435 \u043d\u0430 29 \u044e\u043d\u0438<\/span><\/strong> \u043e\u0442 13:30<\/strong> \u0447\u0430\u0441\u0430 \u0432 \u0437\u0430\u043b\u0430 301<\/strong> \u043d\u0430 \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442\u0430 \u043f\u043e \u0415\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u0438\u043a\u0430 \u043d\u0430 \u0411\u0410\u041d, \u0426\u0430\u0440\u0438\u0433\u0440\u0430\u0434\u0441\u043a\u043e \u0428\u043e\u0441\u0435 72, \u0421\u043e\u0444\u0438\u044f.<\/p>\n \u0422\u0435\u043c\u0430<\/span>: \u201cUltraluminous X-ray sources\u201d<\/strong><\/p>\n \u0414\u043e\u043a\u043b\u0430\u0434\u0432\u0430: prof. DSc Sergei Fabrika<\/strong>, Head of the Laboratory of Stellar Physics at the<\/p>\n Special Astrophysical Observatory of the Russian Academy of Sciences<\/p>\n \u041f\u043e\u043a\u0430\u043d\u0435\u043d\u0438 \u0441\u0430 \u0432\u0441\u0438\u0447\u043a\u0438 \u0438\u043d\u0442\u0435\u0440\u0435\u0441\u0443\u0432\u0430\u0449\u0438 \u0441\u0435.<\/p>\n \u041e\u0442 \u0440\u044a\u043a\u043e\u0432\u043e\u0434\u0441\u0442\u0432\u043e\u0442\u043e \u043d\u0430 \u0441\u0435\u043c\u0438\u043d\u0430\u0440\u0430<\/p>\n \n \u0410\u0431\u0441\u0442\u0440\u0430\u043a\u0442:<\/p>\n The origin of Ultraluminous X-ray sources (ULXs) in external<\/p>\n galaxies whose X-ray luminosities exceed those of the brightest black<\/p>\n holes in our Galaxy by hundreds and thousands of times is mysterious. The<\/p>\n most popular models for the ULXs involve either intermediate mass black<\/p>\n holes (IMBH, ~1000 solar masses) with standard accretion disks or<\/p>\n stellar-mass black holes (10 solar masses) accreting at super-Eddington<\/p>\n rates. We find that all ever spectrally observed ULX counterparts have the<\/p>\n same optical spectra and they are very similar to that of SS 433, the only<\/p>\n known supercritical accretor in Milky Way. We study ULXs in two classical<\/p>\n galactic mergings Antennae and NGC3256. All the ULXs are located nearby<\/p>\n (in 200 pc) or inside extremely young (< 5 Myrs) massive stellar clusters,<\/p>\n and this association is not occasional. The ULX progenitor mass is bigger<\/p>\n than 40-50 solar masses. Probably, these close binary systems were ejected<\/p>\n from the interior of massive-star clusters during the cluster formation.<\/p>\n","protected":false},"excerpt":{"rendered":" \u041d\u0410\u0423\u0427\u0415\u041d \u0421\u0415\u041c\u0418\u041d\u0410\u0420 \u0420\u0435\u0434\u043e\u0432\u043d\u0430\u0442\u0430 \u0441\u0431\u0438\u0440\u043a\u0430 \u043d\u0430 \u0441\u0435\u043c\u0438\u043d\u0430\u0440\u0430 \u043d\u0430 \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442\u0430 \u043f\u043e \u0410\u0441\u0442\u0440\u043e\u043d\u043e\u043c\u0438\u044f \u0449\u0435 \u0441\u0435 \u043f\u0440\u043e\u0432\u0435\u0434\u0435 \u043d\u0430 29 \u044e\u043d\u0438 \u043e\u0442 13:30 \u0447\u0430\u0441\u0430 \u0432 \u0437\u0430\u043b\u0430 301 \u043d\u0430 \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442\u0430 \u043f\u043e \u0415\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u0438\u043a\u0430 \u043d\u0430 \u0411\u0410\u041d, \u0426\u0430\u0440\u0438\u0433\u0440\u0430\u0434\u0441\u043a\u043e \u0428\u043e\u0441\u0435 72, \u0421\u043e\u0444\u0438\u044f. \u0422\u0435\u043c\u0430: \u201cUltraluminous X-ray sources\u201d \u0414\u043e\u043a\u043b\u0430\u0434\u0432\u0430: prof. DSc Sergei Fabrika, Head of the Laboratory of Stellar Physics at the Special Astrophysical Observatory of the […]<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"link","meta":{"footnotes":""},"categories":[10],"tags":[],"class_list":["post-312","post","type-post","status-publish","format-link","hentry","category-10","post_format-post-format-link","category-10-id","post-seq-1","post-parity-odd","meta-position-corners","fix"],"_links":{"self":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts\/312","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=312"}],"version-history":[{"count":1,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts\/312\/revisions"}],"predecessor-version":[{"id":313,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts\/312\/revisions\/313"}],"wp:attachment":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=312"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=312"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=312"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}