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	<title>Comments on: Double dipped supernova</title>
	<atom:link href="http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/</link>
	<description>I am an astronomer, writer, and skeptic. I likes reality the way it is, and I aims to keep it that way. My real name is Phil Plait, and I run the Bad Astronomy blog.</description>
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		<title>By: fwhnpymu rdfiawqmy</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/comment-page-1/#comment-97231</link>
		<dc:creator>fwhnpymu rdfiawqmy</dc:creator>
		<pubDate>Mon, 07 Jul 2008 17:51:46 +0000</pubDate>
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		<description>outjgvz czpj latyk qgylfecz xeqjzuw qwcnoxugm bieavyxrw</description>
		<content:encoded><![CDATA[<p>outjgvz czpj latyk qgylfecz xeqjzuw qwcnoxugm bieavyxrw</p>
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		<title>By: tvuprksqa xiwpem</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/comment-page-1/#comment-97230</link>
		<dc:creator>tvuprksqa xiwpem</dc:creator>
		<pubDate>Mon, 07 Jul 2008 17:48:29 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/#comment-97230</guid>
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		<content:encoded><![CDATA[<p>vrdxynkm ujpoxzwnm qjflm zkpjqbsc bmgwp wsjelabp qfljwhye</p>
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		<title>By: Astrolink [Global Edition] &#187; Astrosphere for June 15, 2007 &#124; Latest astronomy news in 11 languages</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/comment-page-1/#comment-38552</link>
		<dc:creator>Astrolink [Global Edition] &#187; Astrosphere for June 15, 2007 &#124; Latest astronomy news in 11 languages</dc:creator>
		<pubDate>Fri, 15 Jun 2007 19:40:28 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/#comment-38552</guid>
		<description>[...] I covered the double supernova here. Phil Plait from Bad Astronomy has a great description of it was well. [...]</description>
		<content:encoded><![CDATA[<p>[...] I covered the double supernova here. Phil Plait from Bad Astronomy has a great description of it was well. [...]</p>
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		<title>By: Peter Hornby</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/comment-page-1/#comment-38551</link>
		<dc:creator>Peter Hornby</dc:creator>
		<pubDate>Fri, 15 Jun 2007 18:13:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/#comment-38551</guid>
		<description>To be strictly accurate, the previous major outburst of Eta Carinae was in the 1830&#039;s and 1840&#039;s, not the 1870&#039;s.  The star reached magnitude -1 (brighter than Canopus and only half a magnitude down on Sirius) in 1843.</description>
		<content:encoded><![CDATA[<p>To be strictly accurate, the previous major outburst of Eta Carinae was in the 1830&#8217;s and 1840&#8217;s, not the 1870&#8217;s.  The star reached magnitude -1 (brighter than Canopus and only half a magnitude down on Sirius) in 1843.</p>
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		<title>By: JC</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/comment-page-1/#comment-38550</link>
		<dc:creator>JC</dc:creator>
		<pubDate>Fri, 15 Jun 2007 15:05:00 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/#comment-38550</guid>
		<description>Yes, I&#039;m curious as well...what makes you set Eta Car apart from other luminous blue variables? I know little about this, but I thought it was just considered a singularly spectacular example of that class.</description>
		<content:encoded><![CDATA[<p>Yes, I&#8217;m curious as well&#8230;what makes you set Eta Car apart from other luminous blue variables? I know little about this, but I thought it was just considered a singularly spectacular example of that class.</p>
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		<title>By: Astrogeek</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/comment-page-1/#comment-38549</link>
		<dc:creator>Astrogeek</dc:creator>
		<pubDate>Fri, 15 Jun 2007 15:04:27 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/#comment-38549</guid>
		<description>Brian/Gary;

I&#039;m not certain, but I think an abundance of helium is expected because of the sheer size of the H-burning zone in these hyper-massive stars, and because of the upheavals expected in their evolution.

The presence of heavy elements causes these massive stars to blow off mass during the formation phase.  I&#039;m not clear on why that is, but I&#039;ve seen it referenced several times.  Something about the presence of heavy elements making the solar winds more efficient at carving out a hollow in the proto-stellar gas cloud.

Thats also why we think that Pop. III stars could get monstrously huge (perhaps up to about 500Msol) and why that&#039;s not possible in Pop. II or Pop. I stars.</description>
		<content:encoded><![CDATA[<p>Brian/Gary;</p>
<p>I&#8217;m not certain, but I think an abundance of helium is expected because of the sheer size of the H-burning zone in these hyper-massive stars, and because of the upheavals expected in their evolution.</p>
<p>The presence of heavy elements causes these massive stars to blow off mass during the formation phase.  I&#8217;m not clear on why that is, but I&#8217;ve seen it referenced several times.  Something about the presence of heavy elements making the solar winds more efficient at carving out a hollow in the proto-stellar gas cloud.</p>
<p>Thats also why we think that Pop. III stars could get monstrously huge (perhaps up to about 500Msol) and why that&#8217;s not possible in Pop. II or Pop. I stars.</p>
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		<title>By: jackd</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/comment-page-1/#comment-38539</link>
		<dc:creator>jackd</dc:creator>
		<pubDate>Fri, 15 Jun 2007 14:49:14 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/06/14/double-dipped-supernova/#comment-38539</guid>
		<description>I&#039;m missing something here.  What is it that makes Eta Carinae singular?  Its size is amazing, but obviously not unique.  The fact that it blew off so much mass is awe-inspiring, but that&#039;s an effect, not a quality.  So what is it?  I assume we must know something about the two monster stars recently discovered that tells us that they don&#039;t match Eta C - and it wouldn&#039;t just be the lack of an ejected nebula, since that could happen tomorrow, right?

Maybe I&#039;m just reading too much into your statement, but I do feel that you&#039;ve said something I just don&#039;t understand.</description>
		<content:encoded><![CDATA[<p>I&#8217;m missing something here.  What is it that makes Eta Carinae singular?  Its size is amazing, but obviously not unique.  The fact that it blew off so much mass is awe-inspiring, but that&#8217;s an effect, not a quality.  So what is it?  I assume we must know something about the two monster stars recently discovered that tells us that they don&#8217;t match Eta C &#8211; and it wouldn&#8217;t just be the lack of an ejected nebula, since that could happen tomorrow, right?</p>
<p>Maybe I&#8217;m just reading too much into your statement, but I do feel that you&#8217;ve said something I just don&#8217;t understand.</p>
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