Line emission in shocks and PDR - Observatoire de Paris
Line emission in shocks and PDR - Observatoire de Paris
Line emission in shocks and PDR - Observatoire de Paris
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Photo Dissociation Regions<br />
(<strong>PDR</strong>s)<br />
I<strong>de</strong>al laboratories for ISM physical <strong>and</strong> chemical processes<br />
important targets for ALMA <strong>and</strong> Herschel<br />
Herschel :<br />
Cool<strong>in</strong>g processes ([CII], [OI], CO, H 2<br />
O) <strong>and</strong> thermal balance<br />
Chemistry (H 2<br />
O ; C- N- <strong>and</strong> O- hydri<strong>de</strong>s <strong>in</strong>clud<strong>in</strong>g CH + )<br />
Complex molecules (C clusters, PAHs, ...)<br />
Dynamics of the hot <strong>in</strong>terface<br />
Dust properties (from SED)<br />
ALMA : Small scale structures <strong>in</strong> the <strong>in</strong>terface, turbulence, coupl<strong>in</strong>g of<br />
gas dynamics <strong>and</strong> chemistry : time <strong>de</strong>pen<strong>de</strong>nt effects<br />
<strong>L<strong>in</strong>e</strong> <strong>and</strong> cont<strong>in</strong>uum polarisation us<strong>in</strong>g radicals<br />
Dusty04 - <strong>Paris</strong>, October 2004