comparison of gas and dust cooling rates in - Rencontres de Moriond
comparison of gas and dust cooling rates in - Rencontres de Moriond
comparison of gas and dust cooling rates in - Rencontres de Moriond
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E. Bayet<br />
Comparison between differents tracers : 2) Coolants<br />
(neutral <strong>and</strong> molecular <strong>gas</strong> + <strong>dust</strong>)<br />
<strong>Moriond</strong> – March, 6th-12th 2005<br />
Correlations<br />
between<br />
CII, C <strong>and</strong> CO<br />
<strong>cool<strong>in</strong>g</strong> <strong>rates</strong><br />
CII <strong>cool<strong>in</strong>g</strong> rate<br />
> OI <strong>cool<strong>in</strong>g</strong><br />
rate<br />
Starburst galaxies<br />
(NGC 253, M 83)<br />
have the highest<br />
CII, OI, C & CO<br />
<strong>cool<strong>in</strong>g</strong> <strong>rates</strong> <strong>and</strong><br />
highest FIR flux<br />
Merger <strong>and</strong><br />
irregular galaxies<br />
have the lowest <strong>rates</strong>
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