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	<title>Apparent Brightness &#187; AGN</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>Black Hole Growth in Hierarchical Galaxy Formation</title>
		<link>http://apparentbrightness.net/2007/11/07/black-hole-growth-in-hierarchical-galaxy-formation/</link>
		<comments>http://apparentbrightness.net/2007/11/07/black-hole-growth-in-hierarchical-galaxy-formation/#comments</comments>
		<pubDate>Wed, 07 Nov 2007 09:58:01 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

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

		<category><![CDATA[Black Holes]]></category>

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

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

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

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

		<guid isPermaLink="false">http://apparentbrightness.net/2007/11/07/black-hole-growth-in-hierarchical-galaxy-formation/</guid>
		<description><![CDATA[	
		Malbon et al.
		http://arxiv.org/abs/astro-ph/0607424
		Black Hole &#8211; bulge mass relation
		They find that the direct accretion of cold gas during starbursts is an important growth mechanism for lower mass black holes and at high redshift. On the other hand, the re-assembly of pre-existing black hole mass into larger units via merging dominates the growth of more massive black [...]]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>Malbon et al.</li>
		<li><a href="http://arxiv.org/abs/astro-ph/0607424">http://arxiv.org/abs/astro-ph/0607424</a></li>
		<li>Black Hole &#8211; bulge mass relation</li>
		<li>They find that the direct accretion of cold gas during starbursts is an important growth mechanism for lower mass black holes and at high redshift. On the other hand, the re-assembly of pre-existing black hole mass into larger units via merging dominates the growth of more massive black holes at low redshift. </li>
		<li>As redshift decreases, progressively less massive black holes have the highest fractional growth rates, in line with recent claims of &#8220;downsizing&#8221; in quasar activity.</li>
	</ul>

 ]]></content:encoded>
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		<title>Broad Line Emission in Low-Metallicity Blue Compact Dwarf Galaxies: Evidence for Stellar Wind, Supernova and Possible AGN Activity</title>
		<link>http://apparentbrightness.net/2007/10/31/broad-line-emission-in-low-metallicity-blue-compact-dwarf-galaxies-evidence-for-stellar-wind-supernova-and-possible-agn-activity/</link>
		<comments>http://apparentbrightness.net/2007/10/31/broad-line-emission-in-low-metallicity-blue-compact-dwarf-galaxies-evidence-for-stellar-wind-supernova-and-possible-agn-activity/#comments</comments>
		<pubDate>Wed, 31 Oct 2007 14:03:28 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

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

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

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

		<category><![CDATA[H-alpha]]></category>

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

		<guid isPermaLink="false">http://apparentbrightness.net/2007/10/31/broad-line-emission-in-low-metallicity-blue-compact-dwarf-galaxies-evidence-for-stellar-wind-supernova-and-possible-agn-activity/</guid>
		<description><![CDATA[	
		Izotov et al.
		http://arxiv.org/abs/0709.3643
		23 objects, 14 with broad emission
	

 ]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>Izotov et al.</li>
		<li><a href="http://arxiv.org/abs/0709.3643">http://arxiv.org/abs/0709.3643</a></li>
		<li>23 objects, 14 with broad emission</li>
	</ul>

 ]]></content:encoded>
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		</item>
		<item>
		<title>Observational evidence for AGN feedback in early-type galaxies</title>
		<link>http://apparentbrightness.net/2007/10/31/observational-evidence-for-agn-feedback-in-early-type-galaxies/</link>
		<comments>http://apparentbrightness.net/2007/10/31/observational-evidence-for-agn-feedback-in-early-type-galaxies/#comments</comments>
		<pubDate>Wed, 31 Oct 2007 13:40:36 +0000</pubDate>
		<dc:creator>Thomas Marquart</dc:creator>
		
		<category><![CDATA[Paper]]></category>

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

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

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

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

		<guid isPermaLink="false">http://apparentbrightness.net/2007/10/31/observational-evidence-for-agn-feedback-in-early-type-galaxies/</guid>
		<description><![CDATA[	
		Schawinski et al.
		http://arxiv.org/abs/0709.3015
		Sloan study
		morphologically select from &#8220;green valley&#8221;
		star formation history
		time sequence
		quenching
	

 ]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>Schawinski et al.</li>
		<li><a href="http://arxiv.org/abs/0709.3015">http://arxiv.org/abs/0709.3015</a></li>
		<li>Sloan study</li>
		<li>morphologically select from &#8220;green valley&#8221;</li>
		<li>star formation history</li>
		<li>time sequence</li>
		<li>quenching</li>
	</ul>

 ]]></content:encoded>
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