The Excited and Exciting ISM in Galaxies: PDRs, XDRs ... - Caltech
The Excited and Exciting ISM in Galaxies: PDRs, XDRs ... - Caltech
The Excited and Exciting ISM in Galaxies: PDRs, XDRs ... - Caltech
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Conclusions<br />
Future of HerCULES is very excit<strong>in</strong>g<br />
Can dist<strong>in</strong>guish <strong>PDRs</strong>, <strong>XDRs</strong>, CDRs, shocks<br />
With ALMA one can further get:<br />
Dynamical masses <strong>in</strong> NLR <strong>and</strong> BLR<br />
Accretion rates<br />
Edd<strong>in</strong>gton <strong>and</strong> star formation efficiencies<br />
Quantitative measures of local feedback
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