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	<title>Apparent Brightness &#187; UltraViolet</title>
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	<description>astronomy and stuff</description>
	<pubDate>Mon, 03 Dec 2007 16:07:54 +0000</pubDate>
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		<title>The role of minor mergers in the recent star formation history of early-type galaxies</title>
		<link>http://apparentbrightness.net/2007/11/12/the-role-of-minor-mergers-in-the-recent-star-formation-history-of-early-type-galaxies/</link>
		<comments>http://apparentbrightness.net/2007/11/12/the-role-of-minor-mergers-in-the-recent-star-formation-history-of-early-type-galaxies/#comments</comments>
		<pubDate>Mon, 12 Nov 2007 12:14:02 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

		<category><![CDATA[Dwarf]]></category>

		<category><![CDATA[Elliptical]]></category>

		<category><![CDATA[Galaxies]]></category>

		<category><![CDATA[Merger]]></category>

		<category><![CDATA[Simulation]]></category>

		<category><![CDATA[UltraViolet]]></category>

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		<description><![CDATA[	
		Kaviraj et al.
		http://arxiv.org/abs/0711.1493
		Simulations on how minor mergers can explain the variation in UV-fluxes of ellipticals.
		They say they cannot &#8220;rule out&#8221; gas accretion, but I wonder where the dividing line goes between a gas-rich dwarf being eaten and infall of gas.
	

 ]]></description>
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		<li>Kaviraj et al.</li>
		<li><a href="http://arxiv.org/abs/0711.1493">http://arxiv.org/abs/0711.1493</a></li>
		<li>Simulations on how minor mergers can explain the variation in UV-fluxes of ellipticals.</li>
		<li>They say they cannot &#8220;rule out&#8221; gas accretion, but I wonder where the dividing line goes between a gas-rich dwarf being eaten and infall of gas.</li>
	</ul>

 ]]></content:encoded>
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		<title>The UV properties of E+A galaxies: constraints on feedback-driven quenching of star formation</title>
		<link>http://apparentbrightness.net/2007/11/05/the-uv-properties-of-ea-galaxies-constraints-on-feedback-driven-quenching-of-star-formation/</link>
		<comments>http://apparentbrightness.net/2007/11/05/the-uv-properties-of-ea-galaxies-constraints-on-feedback-driven-quenching-of-star-formation/#comments</comments>
		<pubDate>Mon, 05 Nov 2007 07:04:25 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

		<category><![CDATA[Galaxies]]></category>

		<category><![CDATA[Postburst]]></category>

		<category><![CDATA[Quenching]]></category>

		<category><![CDATA[Star Formation]]></category>

		<category><![CDATA[Starburst]]></category>

		<category><![CDATA[UltraViolet]]></category>

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		<description><![CDATA[	
		Kaviraj et al.
		http://arxiv.org/abs/0707.3570
		postburst galaxies and quenching of star-formation
		connection to ULIRGs
	

 ]]></description>
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		<li>Kaviraj et al.</li>
		<li><a href="http://arxiv.org/abs/0707.3570">http://arxiv.org/abs/0707.3570</a></li>
		<li>postburst galaxies and quenching of star-formation</li>
		<li>connection to ULIRGs</li>
	</ul>

 ]]></content:encoded>
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