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	<title>Apparent Brightness &#187; Feedback</title>
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	<link>http://apparentbrightness.net</link>
	<description>astronomy and stuff</description>
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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</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>
	</ul>
	<ul>
		<li>23 objects, 14 with broad emission</li>
	</ul>

 ]]></content:encoded>
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		<slash:comments>0</slash:comments>
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		<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</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>
	</ul>
	<ul>
		<li>quenching</li>
	</ul>

 ]]></content:encoded>
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		<title>Outflow or galactic wind: The fate of ionized gas in the halos of dwarf galaxies</title>
		<link>http://apparentbrightness.net/2007/10/31/outflow-or-galactic-wind-the-fate-of-ionized-gas-in-the-halos-of-dwarf-galaxies/</link>
		<comments>http://apparentbrightness.net/2007/10/31/outflow-or-galactic-wind-the-fate-of-ionized-gas-in-the-halos-of-dwarf-galaxies/#comments</comments>
		<pubDate>Wed, 31 Oct 2007 13:31:15 +0000</pubDate>
		<dc:creator>Thomas</dc:creator>
				<category><![CDATA[Paper]]></category>
		<category><![CDATA[Feedback]]></category>
		<category><![CDATA[Galaxies]]></category>
		<category><![CDATA[H-alpha]]></category>
		<category><![CDATA[Kinematics]]></category>
		<category><![CDATA[Starburst]]></category>

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		<description><![CDATA[Eymeren et al. http://arxiv.org/abs/0709.2974 extended H-alpha emssion around starbursts deep narrow-band images &#038; slit spectra of NGC 2366 and NGC 4861 outflows]]></description>
			<content:encoded><![CDATA[	<ul>
		<li>Eymeren et al.</li>
		<li><a href="http://arxiv.org/abs/0709.2974">http://arxiv.org/abs/0709.2974</a></li>
		<li>extended H-alpha emssion around starbursts</li>
		<li>deep narrow-band images &#038; slit spectra of NGC 2366 and NGC 4861</li>
	</ul>
	<ul>
		<li>outflows</li>
	</ul>

 ]]></content:encoded>
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		<slash:comments>0</slash:comments>
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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</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>

		<guid isPermaLink="false">http://apparentbrightness.net/2007/10/31/scaling-relations-of-dwarf-galaxies-without-supernova-driven-winds/</guid>
		<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>
	</ul>
	<ul>
		<li>useful to compare to where our data fall on these correlations</li>
	</ul>

 ]]></content:encoded>
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