{"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":"K. Leighly - Understanding Broad Absorption Line Quasars - AGN Driven Winds","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"W6bpRKu7R5\"><a href=\"https:\/\/phsites.technion.ac.il\/agn-2017\/k-leighly-understanding-broad-absorption-line-quasars\/\">K. Leighly &#8211; Understanding Broad Absorption Line Quasars<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/phsites.technion.ac.il\/agn-2017\/k-leighly-understanding-broad-absorption-line-quasars\/embed\/#?secret=W6bpRKu7R5\" width=\"600\" height=\"338\" title=\"&#8220;K. Leighly &#8211; Understanding Broad Absorption Line Quasars&#8221; &#8212; AGN Driven Winds\" data-secret=\"W6bpRKu7R5\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\" class=\"wp-embedded-content\"><\/iframe><script>\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<\/script>\n","description":"Despite decades of study, broad absorption line quasars are poorly understood. For example, we know that partial covering is important, but what is the physical nature of partial covering? Many of these questions stem from the fact that the spectra are very difficult to analyze, principally as a consequence of blending and problems constraining the &hellip;"}