{"type":"video","version":"1.0","provider_name":"Network.hu","provider_url":"http:\/\/network.hu\/","title":"Nasa Quasar Animation","author_name":"nagi18","author_url":"http:\/\/network.hu\/nagi18","html":"<object width="424" height="345"><param name="movie" value="http:\/\/vilagur.network.hu\/flash\/videoplayer\/video.swf?videoid=72265&pvol=40&plang=hu&host=http:\/\/vilagur.network.hu" \/><param name="allowscriptaccess" value="always" \/><param name="allowfullscreen" value="true" \/><embed src="http:\/\/vilagur.network.hu\/flash\/videoplayer\/video.swf?videoid=72265&pvol=40&plang=hu&host=http:\/\/vilagur.network.hu" width="424" height="345" allowscriptaccess="always" allowfullscreen="true" \/><\/object>","width":424,"height":345,"description":"csillagszer\u0171 (azaz kv\u00e1zisztell\u00e1ris) r\u00e1di\u00f3forr\u00e1s. A kvaz\u00e1rok \u00e1ltal\u00e1ban nagy v\u00f6r\u00f6seltol\u00f3d\u00e1s\u00fa, t\u00e1voli galaxisok akt\u00edv magjai, leggyakoribbak az \u0150srobban\u00e1s ut\u00e1n 2-3 milli\u00e1rd \u00e9vvel voltak. Energiakibocs\u00e1t\u00e1suk er\u0151sen v\u00e1ltozik, \u00e1ltal\u00e1ban kb. t\u00edzezerszerese a Tej\u00fatrendszer\u00e9nek, f\u0151k\u00e9nt nagyenergi\u00e1j\u00fa sug\u00e1rz\u00e1sb\u00f3l \u00e1ll. Az aktivit\u00e1st egy \u00f3ri\u00e1si t\u00f6meg\u0171 k\u00f6zponti fekete lyuk hozza l\u00e9tre, amelybe k\u00f6rnyezet\u00e9b\u0151l anyag \u00e1ramlik egy akkr\u00e9ci\u00f3s korongon kereszt\u00fcl. A kvaz\u00e1rokn\u00e1l ennek a korongnak a s\u00edkj\u00e1ra kb. 90-45 fokos sz\u00f6g k\u00f6z\u00f6tt l\u00e1tunk r\u00e1. Amikor egy kvaz\u00e1rn\u00e1l a heves folyamatok al\u00e1bbhagynak, aktivit\u00e1sa megsz\u0171nik, \"norm\u00e1lis\" galaxismag lesz bel\u0151le.","thumbnail_url":"http:\/\/vds.network.hu\/clubvideo\/7\/2\/_\/72265_834215_2.jpg","thumbnail_width":80,"thumbnail_height":60,"video_id":"72265"}