<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:wfw="http://wellformedweb.org/CommentAPI/"
	xmlns:dc="http://purl.org/dc/elements/1.1/"
	xmlns:atom="http://www.w3.org/2005/Atom"
	>

<channel>
	<title>Apparent Brightness &#187; Merger</title>
	<atom:link href="http://apparentbrightness.net/tag/merger/feed/" rel="self" type="application/rss+xml" />
	<link>http://apparentbrightness.net</link>
	<description>astronomy and stuff</description>
	<pubDate>Mon, 03 Dec 2007 16:07:54 +0000</pubDate>
	<generator>http://wordpress.org/?v=2.6</generator>
	<language>en</language>
			<item>
		<title>Star-formation in the HI bridge between M81 and M82</title>
		<link>http://apparentbrightness.net/2007/11/20/star-formation-in-the-hi-bridge-between-m81-and-m82/</link>
		<comments>http://apparentbrightness.net/2007/11/20/star-formation-in-the-hi-bridge-between-m81-and-m82/#comments</comments>
		<pubDate>Tue, 20 Nov 2007 14:13:50 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

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

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

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

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

		<category><![CDATA[Stellar Populations]]></category>

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

		<guid isPermaLink="false">http://apparentbrightness.net/2007/11/20/star-formation-in-the-hi-bridge-between-m81-and-m82/</guid>
		<description><![CDATA[	
		de Mello et al.
		http://arxiv.org/abs/0711.2685
		They found both old and young stars in the region between the two galaxies and conclude that the former were flung out of either of the two while the latter have formed in the tidal tail.
		Overall, there seems to be quite little going on there compared to other tidal tails (e.g. of [...]]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>de Mello et al.</li>
		<li><a href="http://arxiv.org/abs/0711.2685">http://arxiv.org/abs/0711.2685</a></li>
		<li>They found both old and young stars in the region between the two galaxies and conclude that the former were flung out of either of the two while the latter have formed in the tidal tail.</li>
		<li>Overall, there seems to be quite little going on there compared to other tidal tails (e.g. of mergers) where active star formation is often seen.</li>
	</ul>

 ]]></content:encoded>
			<wfw:commentRss>http://apparentbrightness.net/2007/11/20/star-formation-in-the-hi-bridge-between-m81-and-m82/feed/</wfw:commentRss>
		</item>
		<item>
		<title>The MW is an exceptionnally quiet galaxy: implications for spiral formation</title>
		<link>http://apparentbrightness.net/2007/11/20/the-mw-is-an-exceptionnally-quiet-galaxy-implications-for-spiral-formation/</link>
		<comments>http://apparentbrightness.net/2007/11/20/the-mw-is-an-exceptionnally-quiet-galaxy-implications-for-spiral-formation/#comments</comments>
		<pubDate>Tue, 20 Nov 2007 14:06:40 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

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

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

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

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

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

		<guid isPermaLink="false">http://apparentbrightness.net/2007/11/20/the-mw-is-an-exceptionnally-quiet-galaxy-implications-for-spiral-formation/</guid>
		<description><![CDATA[	
		Puech et al.
		http://arxiv.org/abs/0711.2881
		Conference proceeding on how the MW is special in the sense that it forms little stars and therefore cannot have undergone a merger for a long time.
	

 ]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>Puech et al.</li>
		<li><a href="http://arxiv.org/abs/0711.2881">http://arxiv.org/abs/0711.2881</a></li>
		<li>Conference proceeding on how the MW is special in the sense that it forms little stars and therefore cannot have undergone a merger for a long time.</li>
	</ul>

 ]]></content:encoded>
			<wfw:commentRss>http://apparentbrightness.net/2007/11/20/the-mw-is-an-exceptionnally-quiet-galaxy-implications-for-spiral-formation/feed/</wfw:commentRss>
		</item>
		<item>
		<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>

		<guid isPermaLink="false">http://apparentbrightness.net/2007/11/12/the-role-of-minor-mergers-in-the-recent-star-formation-history-of-early-type-galaxies/</guid>
		<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>
			<wfw:commentRss>http://apparentbrightness.net/2007/11/12/the-role-of-minor-mergers-in-the-recent-star-formation-history-of-early-type-galaxies/feed/</wfw:commentRss>
		</item>
		<item>
		<title>2-Dimensional Kinematics of Simulated Disc Merger Remnants</title>
		<link>http://apparentbrightness.net/2007/10/31/2-dimensional-kinematics-of-simulated-disc-merger-remnants/</link>
		<comments>http://apparentbrightness.net/2007/10/31/2-dimensional-kinematics-of-simulated-disc-merger-remnants/#comments</comments>
		<pubDate>Wed, 31 Oct 2007 14:43:27 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

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

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

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

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

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

		<guid isPermaLink="false">http://apparentbrightness.net/2007/10/31/2-dimensional-kinematics-of-simulated-disc-merger-remnants/</guid>
		<description><![CDATA[	
		Jesseit et al.
		http://arxiv.org/abs/astro-ph/0606144
		&#8220;real&#8221; simulations are the way to go for understanding the complex velocity fields of our BCGs.
	

 ]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>Jesseit et al.</li>
		<li><a href="http://arxiv.org/abs/astro-ph/0606144">http://arxiv.org/abs/astro-ph/0606144</a></li>
		<li>&#8220;real&#8221; simulations are the way to go for understanding the complex velocity fields of our BCGs.</li>
	</ul>

 ]]></content:encoded>
			<wfw:commentRss>http://apparentbrightness.net/2007/10/31/2-dimensional-kinematics-of-simulated-disc-merger-remnants/feed/</wfw:commentRss>
		</item>
	</channel>
</rss>
