<?xml version="1.0" encoding="windows-1251" ?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom">
<channel>
<title>Astronet</title>
<description>Latest www.astronet.ru publications</description>
<link>http://www.astronet.ru/</link>
<language>en</language>
<pubDate>Wed, 16 May 2012 00:00:00 GMT</pubDate>
<lastBuildDate>Wed, 16 May 2012 05:30:08 GMT</lastBuildDate>
<docs>http://blogs.law.harvard.edu/tech/rss</docs>
<managingEditor>info@astronet.ru</managingEditor>
<webMaster>info@astronet.ru</webMaster>
<image>
  <title>Astronet</title>
  <url>http://images.astronet.ru/img/logo/astronet.jpg</url>
  <link>http://www.astronet.ru/</link>
  <width>79</width>
  <height>52</height>
</image>

<item>
  <title>Star Formation in the Tarantula Nebula</title>
  <link>http://www.astronet.ru/db/msg/1264606/</link>
  <description><![CDATA[<a href="/db/msg/1264606"><img src="http://images.astronet.ru/pubd/2012/05/16/0001264606/tarantula2_hst_960.preview.jpg" class="title" width="150" height="122" border="1" vspace="3" hspace="10" alt="Star Formation in the Tarantula Nebula" align="right"></a>
The largest, most violent star forming region known in the whole  
Local Group of galaxies  
lies in our neighboring galaxy the  
Large Magellanic Cloud (LMC).  
 
Were the Tarantula Nebula at the distance of the  
Orion Nebula -- a local star forming region --  
it would take up fully half the sky.
]]></description>
  <pubDate>Wed, 16 May 2012 05:30:08 GMT</pubDate>
</item>

<atom:link href="http://www.astronet.ru/db/rss.xml" rel="self" type="application/rss+xml" />
</channel>
</rss>


