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> <channel><title>Comments on: The Strange Case of Supernova SN2008ha</title> <atom:link href="http://www.universetoday.com/2009/06/09/the-strange-case-of-supernova-sn2008ha/feed/" rel="self" type="application/rss+xml" /><link>http://www.universetoday.com/2009/06/09/the-strange-case-of-supernova-sn2008ha/</link> <description>Space and astronomy news</description> <lastBuildDate>Mon, 22 Mar 2010 03:02:27 +0000</lastBuildDate> <generator>http://wordpress.org/?v=2.9.2</generator> <sy:updatePeriod>hourly</sy:updatePeriod> <sy:updateFrequency>1</sy:updateFrequency> <item><title>By: Jon Hanford</title><link>http://www.universetoday.com/2009/06/09/the-strange-case-of-supernova-sn2008ha/comment-page-1/#comment-67338</link> <dc:creator>Jon Hanford</dc:creator> <pubDate>Fri, 12 Jun 2009 00:36:29 +0000</pubDate> <guid
isPermaLink="false">http://www.universetoday.com/?p=32219#comment-67338</guid> <description>As if this type of peculiar supernova weren&#039;t enough, researchers just posted an eprint entitled &quot;A new type of stellar explosion&quot; discussing an underluminous Type Ib supernova in the galaxy NGC 1032 back in 2005. The paper can be found here: http://arxiv.org/abs/0906.2003 . Some similarities between it (SN 2005E) and SN 2008ha are mentioned in the paper.</description> <content:encoded><![CDATA[<p>As if this type of peculiar supernova weren&#039;t enough, researchers just posted an eprint entitled &#034;A new type of stellar explosion&#034; discussing an underluminous Type Ib supernova in the galaxy NGC 1032 back in 2005. The paper can be found here: <a
href="http://arxiv.org/abs/0906.2003" rel="nofollow">http://arxiv.org/abs/0906.2003</a> . Some similarities between it (SN 2005E) and SN 2008ha are mentioned in the paper.</p> ]]></content:encoded> </item> <item><title>By: Jon Hanford</title><link>http://www.universetoday.com/2009/06/09/the-strange-case-of-supernova-sn2008ha/comment-page-1/#comment-67336</link> <dc:creator>Jon Hanford</dc:creator> <pubDate>Thu, 11 Jun 2009 21:57:11 +0000</pubDate> <guid
isPermaLink="false">http://www.universetoday.com/?p=32219#comment-67336</guid> <description>A second paper by an independent team of researchers is available here: http://arxiv.org/abs/0902.2794v2 . @jimmNJ, I think that Type Ia supernovae were used to infer the existence of Dark Energy, so these underluminous Type II supernovae should not alter the evidence for DE.</description> <content:encoded><![CDATA[<p>A second paper by an independent team of researchers is available here: <a
href="http://arxiv.org/abs/0902.2794v2" rel="nofollow">http://arxiv.org/abs/0902.2794v2</a> . @jimmNJ, I think that Type Ia supernovae were used to infer the existence of Dark Energy, so these underluminous Type II supernovae should not alter the evidence for DE.</p> ]]></content:encoded> </item> <item><title>By: jimmNJ</title><link>http://www.universetoday.com/2009/06/09/the-strange-case-of-supernova-sn2008ha/comment-page-1/#comment-67250</link> <dc:creator>jimmNJ</dc:creator> <pubDate>Wed, 10 Jun 2009 19:14:41 +0000</pubDate> <guid
isPermaLink="false">http://www.universetoday.com/?p=32219#comment-67250</guid> <description>Could this affect the calculation of Dark Energy using supernovae luminosities?</description> <content:encoded><![CDATA[<p>Could this affect the calculation of Dark Energy using supernovae luminosities?</p> ]]></content:encoded> </item> <item><title>By: Jon Hanford</title><link>http://www.universetoday.com/2009/06/09/the-strange-case-of-supernova-sn2008ha/comment-page-1/#comment-67176</link> <dc:creator>Jon Hanford</dc:creator> <pubDate>Tue, 09 Jun 2009 18:35:42 +0000</pubDate> <guid
isPermaLink="false">http://www.universetoday.com/?p=32219#comment-67176</guid> <description>I was at first curious as to how the researchers accounted for internal galactic absorption in this particular supernova. Upon reading a copy of the preprint: http://arxiv.org/abs/0901.2074v2 .  I see they found very little intrinsic absorption in this galaxy. The paper also brings up implications for nearby long GRBs and has several other peculiar SNe highlighted. Unusually dim luminosity coupled with missing hydrogen lines rightly needs to be adequately explained.</description> <content:encoded><![CDATA[<p>I was at first curious as to how the researchers accounted for internal galactic absorption in this particular supernova. Upon reading a copy of the preprint: <a
href="http://arxiv.org/abs/0901.2074v2" rel="nofollow">http://arxiv.org/abs/0901.2074v2</a> .  I see they found very little intrinsic absorption in this galaxy. The paper also brings up implications for nearby long GRBs and has several other peculiar SNe highlighted. Unusually dim luminosity coupled with missing hydrogen lines rightly needs to be adequately explained.</p> ]]></content:encoded> </item> </channel> </rss>
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