{"version":"1.0","provider_name":"Prof. Noam Soker","provider_url":"https:\/\/phsites.technion.ac.il\/soker","author_name":"Noam Soker","author_url":"https:\/\/phsites.technion.ac.il\/soker\/author\/nsoker\/","title":"Forming equatorial rings around dying stars (March 2015) Prof. Noam Soker","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"Msi0TlIdj4\"><a href=\"https:\/\/phsites.technion.ac.il\/soker\/forming-equatorial-rings-around-dying-stars\/\">Forming equatorial rings around dying stars (March 2015)<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/phsites.technion.ac.il\/soker\/forming-equatorial-rings-around-dying-stars\/embed\/#?secret=Msi0TlIdj4\" width=\"600\" height=\"338\" title=\"&#8220;Forming equatorial rings around dying stars (March 2015)&#8221; &#8212; Prof. Noam Soker\" data-secret=\"Msi0TlIdj4\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\" class=\"wp-embedded-content\"><\/iframe><script type=\"text\/javascript\">\n\/* <![CDATA[ *\/\n\/*! This file is auto-generated *\/\n!function(d,l){\"use strict\";l.querySelector&&d.addEventListener&&\"undefined\"!=typeof URL&&(d.wp=d.wp||{},d.wp.receiveEmbedMessage||(d.wp.receiveEmbedMessage=function(e){var t=e.data;if((t||t.secret||t.message||t.value)&&!\/[^a-zA-Z0-9]\/.test(t.secret)){for(var s,r,n,a=l.querySelectorAll('iframe[data-secret=\"'+t.secret+'\"]'),o=l.querySelectorAll('blockquote[data-secret=\"'+t.secret+'\"]'),c=new RegExp(\"^https?:$\",\"i\"),i=0;i<o.length;i++)o[i].style.display=\"none\";for(i=0;i<a.length;i++)s=a[i],e.source===s.contentWindow&&(s.removeAttribute(\"style\"),\"height\"===t.message?(1e3<(r=parseInt(t.value,10))?r=1e3:~~r<200&&(r=200),s.height=r):\"link\"===t.message&&(r=new URL(s.getAttribute(\"src\")),n=new URL(t.value),c.test(n.protocol))&&n.host===r.host&&l.activeElement===s&&(d.top.location.href=t.value))}},d.addEventListener(\"message\",d.wp.receiveEmbedMessage,!1),l.addEventListener(\"DOMContentLoaded\",function(){for(var e,t,s=l.querySelectorAll(\"iframe.wp-embedded-content\"),r=0;r<s.length;r++)(t=(e=s[r]).getAttribute(\"data-secret\"))||(t=Math.random().toString(36).substring(2,12),e.src+=\"#?secret=\"+t,e.setAttribute(\"data-secret\",t)),e.contentWindow.postMessage({message:\"ready\",secret:t},\"*\")},!1)))}(window,document);\n\/\/# sourceURL=https:\/\/phsites.technion.ac.il\/soker\/wp-includes\/js\/wp-embed.min.js\n\/* ]]> *\/\n<\/script>\n","description":"Muhammad Akashi, Efrat Sabach, Ohad Yogev and I\u00a0suggest that clumpy-dense outflowing equatorial rings\u00a0around evolved giant stars,\u00a0such as in supernova 1987A and the Necklace planetary nebula, are formed by bipolar jets\u00a0that compress gas toward the equatorial plane. The jets are launched from an accretion disk around a stellar companion.\u00a0The jets account also for the presence of &hellip;","thumbnail_url":"http:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/02\/zAkashi2015.jpg"}