{"version":"1.0","provider_name":"AGN Driven Winds","provider_url":"https:\/\/phsites.technion.ac.il\/agn-2017","author_name":"Adi","author_url":"https:\/\/phsites.technion.ac.il\/agn-2017\/author\/adile\/","title":"S. Aalto - Molecular outflows in AGNs and starbursts - AGN Driven Winds","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"kbOSontfgi\"><a href=\"https:\/\/phsites.technion.ac.il\/agn-2017\/s-aalto-molecular-outflows-agns-starbursts\/\">S. Aalto &#8211; Molecular outflows in AGNs and starbursts<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/phsites.technion.ac.il\/agn-2017\/s-aalto-molecular-outflows-agns-starbursts\/embed\/#?secret=kbOSontfgi\" width=\"600\" height=\"338\" title=\"&#8220;S. Aalto &#8211; Molecular outflows in AGNs and starbursts&#8221; &#8212; AGN Driven Winds\" data-secret=\"kbOSontfgi\" 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\/agn-2017\/wp-includes\/js\/wp-embed.min.js\n\/* ]]> *\/\n<\/script>\n","description":"See Presentation Can AGN-powered molecular jets appear as disk-winds similar to what we see in protostars? If so \u2013 will we then see molecular jets also in the quasar mode of accretion? Is it possible that molecular jets are important processes in solving the angular momentum problem for SMBH growth \u2013 or is the jet &hellip;"}