{"id":743,"date":"2015-01-31T19:42:27","date_gmt":"2015-01-31T19:42:27","guid":{"rendered":"http:\/\/phsites.technion.ac.il\/soker\/?p=743"},"modified":"2015-01-31T20:10:42","modified_gmt":"2015-01-31T20:10:42","slug":"formation-scenario-triple-pulsar-psr-j03371715-january-2015","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/soker\/formation-scenario-triple-pulsar-psr-j03371715-january-2015\/","title":{"rendered":"A formation scenario for the triple pulsar PSR J0337+1715 (January 2015)"},"content":{"rendered":"<p><strong><a href=\"http:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/01\/zPSRJ0337.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"alignright wp-image-749\" src=\"http:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/01\/zPSRJ0337.jpg\" alt=\"zPSRJ0337\" width=\"170\" height=\"240\" srcset=\"https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/01\/zPSRJ0337.jpg 1654w, https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/01\/zPSRJ0337-212x300.jpg 212w, https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/01\/zPSRJ0337-724x1024.jpg 724w\" sizes=\"auto, (max-width: 170px) 100vw, 170px\" \/><\/a>Efrat Sabach<\/strong> and I proposed a scenario for the formation of the pulsar with two white dwarfs (WDs)\u00a0triple system PSR J0337+1715 where a close binary system is tidally and frictionally\u00a0destroyed inside the envelope of a massive star that later goes through an accretion induced\u00a0collapse (AIC) and forms the neutron star (NS). The proposed scenario includes\u00a0<span style=\"background-color: #ffff00\">a new ingredient of a binary system that breaks-up inside a common envelope,<\/span>\u00a0employs\u00a0an efficient envelope removal by jets launched by the compact object immersed in the\u00a0giant envelope, and the <span style=\"background-color: #cc99ff\">newly proposed grazing envelope evolution<\/span>.<\/p>\n<p><a title=\"Paper\" href=\"http:\/\/arxiv.org\/abs\/1501.06787\">Paper<\/a> was posted on astro-ph.\u00a0<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Efrat Sabach and I proposed a scenario for the formation of the pulsar with two white dwarfs (WDs)\u00a0triple system PSR J0337+1715 where a close binary system is tidally and frictionally\u00a0destroyed inside the envelope of a massive star that later goes through an accretion induced\u00a0collapse (AIC) and forms the neutron star (NS). The proposed scenario includes\u00a0a &hellip;<\/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-743","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-news","7":"entry"},"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.5 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>A formation scenario for the triple pulsar PSR J0337+1715 (January 2015) Prof. Noam Soker<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/phsites.technion.ac.il\/soker\/formation-scenario-triple-pulsar-psr-j03371715-january-2015\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"A formation scenario for the triple pulsar PSR J0337+1715 (January 2015) Prof. Noam Soker\" \/>\n<meta property=\"og:description\" content=\"Efrat Sabach and I proposed a scenario for the formation of the pulsar with two white dwarfs (WDs)\u00a0triple system PSR J0337+1715 where a close binary system is tidally and frictionally\u00a0destroyed inside the envelope of a massive star that later goes through an accretion induced\u00a0collapse (AIC) and forms the neutron star (NS). The proposed scenario includes\u00a0a &hellip;\" \/>\n<meta property=\"og:url\" content=\"https:\/\/phsites.technion.ac.il\/soker\/formation-scenario-triple-pulsar-psr-j03371715-january-2015\/\" \/>\n<meta property=\"og:site_name\" content=\"Prof. Noam Soker\" \/>\n<meta property=\"article:published_time\" content=\"2015-01-31T19:42:27+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2015-01-31T20:10:42+00:00\" \/>\n<meta property=\"og:image\" content=\"http:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/01\/zPSRJ0337.jpg\" \/>\n<meta name=\"author\" content=\"Noam Soker\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"Noam Soker\" \/>\n\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"1 minute\" \/>\n<script type=\"application\/ld+json\" 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