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	<title>Apparent Brightness &#187; Dwarf</title>
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	<link>http://apparentbrightness.net</link>
	<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>
			<content:encoded><![CDATA[	<ul>
		<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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		<item>
		<title>Scaling Relations of Dwarf Galaxies without Supernova-Driven Winds</title>
		<link>http://apparentbrightness.net/2007/10/31/scaling-relations-of-dwarf-galaxies-without-supernova-driven-winds/</link>
		<comments>http://apparentbrightness.net/2007/10/31/scaling-relations-of-dwarf-galaxies-without-supernova-driven-winds/#comments</comments>
		<pubDate>Wed, 31 Oct 2007 13:18:27 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

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

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

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

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

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

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

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

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		<description><![CDATA[	
		Tassis et al.
		http://arxiv.org/abs/astro-ph/0609763
		Dwarf galaxies: correlations between their global stellar and dynamical properties, such as circular velocity, mass-to-light ratio, stellar mass, surface brightness, and metallicity.
		low and high z
		simulation work
		SN winds vs. ineficient SF
		useful to compare to where our data fall on these correlations
	

 ]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>Tassis et al.</li>
		<li><a href="http://arxiv.org/abs/astro-ph/0609763">http://arxiv.org/abs/astro-ph/0609763</a></li>
		<li>Dwarf galaxies: correlations between their global stellar and dynamical properties, such as circular velocity, mass-to-light ratio, stellar mass, surface brightness, and metallicity.</li>
		<li>low and high z</li>
		<li>simulation work</li>
		<li>SN winds vs. ineficient SF</li>
		<li>useful to compare to where our data fall on these correlations</li>
	</ul>

 ]]></content:encoded>
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