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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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<strong>The</strong> Molecular Fraction: Resolution Effects<br />

Black pluses: total gas surface density<br />

(correct for <strong>in</strong>cl<strong>in</strong>ation <strong>and</strong> the present<br />

of helium)<br />

+ 7 arcsec <strong>HI</strong> <strong>and</strong> CO maps<br />

+ <strong>HI</strong> <strong>and</strong> CO maps smoothed to 15<br />

arcsec resolution<br />

+ 7 arcsec CO map <strong>and</strong> <strong>HI</strong> maps<br />

smoothed to 15 arcsec<br />

Dash-dot l<strong>in</strong>e: Elmegreen 1993 photodissociation<br />

model with U0=Z0=1<br />

Robust to Resolution!<br />

28

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