The HI-H 2 Transition and Star Formation in Early-Type Galaxies

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Koyama & Ostriker 2008 ---->

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Koyama & Ostriker 2008 ----> 24

Rmol-Pressure Relation •Early-type empirical result: P=[(P/k B )/5200±400 K cm -3 )] 0.45±0.09 •The Elmegreen (1993) prediction, F mol ≈P 2.2 j(Z) -1 , is only good for R mol

Page 1 and 2: The giant elliptical galaxy ESO 325
Page 3 and 4: Motivation It is well known that m
Page 5 and 6: Results NGC 807 Five Detections: N
Page 7 and 8: HI detected HI non-detected UGC 150
Page 9 and 10: Σcrit Versus Σtot
Page 11 and 12: Rmol-Pressure Relation Recall that
Page 13 and 14: Blitz & Rosolowsky 2006; Leroy et a
Page 15 and 16: ρs is constant over Hg? s>>Hg H Ko
Page 17 and 18: ρs is constant over Hg? s>>Hg H Az
Page 19 and 20: ρ s Constant with H g ? The MGE st
Page 21 and 22: Koyama & Ostriker 2008 ----> Hg: 5-
Page 23: Koyama & Ostriker 2008 ----> 23 Gas
Page 27 and 28: Summary • Observed HI surface den

The HI-H 2 Transition and Star Formation in Early-Type Galaxies

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