The HI-H 2 Transition and Star Formation in Early-Type Galaxies
The HI-H 2 Transition and Star Formation in Early-Type Galaxies
The HI-H 2 Transition and Star Formation in Early-Type Galaxies
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Rmol-Pressure Relation<br />
•<strong>Early</strong>-type empirical result: P=[(P/k B<br />
)/5200±400 K cm -3 )] 0.45±0.09<br />
•<strong>The</strong> Elmegreen (1993) prediction, F mol<br />
≈P 2.2 j(Z) -1 , is only good for R mol<br />
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