{"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":"A binary model for the large outburst of SN2009ip (August 2013) Prof. Noam Soker","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"mUofWR5XR9\"><a href=\"https:\/\/phsites.technion.ac.il\/soker\/latest-large-outburst-sn2009ip\/\">A binary model for the large outburst of SN2009ip (August 2013)<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/phsites.technion.ac.il\/soker\/latest-large-outburst-sn2009ip\/embed\/#?secret=mUofWR5XR9\" width=\"600\" height=\"338\" title=\"&#8220;A binary model for the large outburst of SN2009ip (August 2013)&#8221; &#8212; Prof. Noam Soker\" data-secret=\"mUofWR5XR9\" 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":"There is an ongoing debate regarding the nature of the SN impostor SN 2009ip and\u00a0the several outbursts that followed its 2009 eruption (see post below from December 2012). Most controversial is the nature of\u00a0the 2012b outburst, with three main types of scenarios: SN explosion, non-terminal single star\u00a0eruption, and a binary interaction. Recently we further developed &hellip;"}