{"id":1742,"date":"2021-04-26T09:18:37","date_gmt":"2021-04-26T06:18:37","guid":{"rendered":"https:\/\/phsites.technion.ac.il\/soker\/?p=1742"},"modified":"2021-04-26T09:19:11","modified_gmt":"2021-04-26T06:19:11","slug":"double-common-envelope-jets-supernovae-cejsne-by-triple-star-systems-april-2021","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/soker\/double-common-envelope-jets-supernovae-cejsne-by-triple-star-systems-april-2021\/","title":{"rendered":"Double common envelope jets supernovae (CEJSNe) by triple-star systems (April 2021)"},"content":{"rendered":"\n

I propose a new type of common envelope jets supernova (CEJSN) events where instead of a single neutron star (NS; or a black hole; BH) a tight binary system of a NS and a main sequence star enters a common envelope evolution (CEE) with a red supergiant (for the paper<\/a>).  <\/p>\n\n\n\n

\"\"<\/a><\/figure>\n","protected":false},"excerpt":{"rendered":"

I propose a new type of common envelope jets supernova (CEJSN) events where instead of a single neutron star (NS; or a black hole; BH) a tight binary system of a NS and a main sequence star enters a common envelope evolution (CEE) with a red supergiant (for the paper).  <\/p>\n","protected":false},"author":6,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"categories":[2],"tags":[],"class_list":{"0":"post-1742","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-news","7":"entry"},"yoast_head":"\nDouble common envelope jets supernovae (CEJSNe) by triple-star systems (April 2021) Prof. Noam Soker<\/title>\n<meta name=\"robots\" content=\"index, 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