Line emission in shocks and PDR - Observatoire de Paris

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Photo Dissociation Regions (PDRs) Ideal laboratories for ISM physical and chemical processes important targets for ALMA and Herschel Herschel : Cooling processes ([CII], [OI], CO, H 2 O) and thermal balance Chemistry (H 2 O ; C- N- and O- hydrides including CH + ) Complex molecules (C clusters, PAHs, ...) Dynamics of the hot interface Dust properties (from SED) ALMA : Small scale structures in the interface, turbulence, coupling of gas dynamics and chemistry : time dependent effects Line and continuum polarisation using radicals Dusty04 - Paris, October 2004
C x B x B" x A x A" x C" x ODIN beams in IRAS 16293 outflow on CO map of Lis et al.(2002)
Page 1 and 2: Line emission from shocks Sylvie Ca
Page 3 and 4: Evidence for C-precursors: H2 pure
Page 5 and 6: Shocks sampled by ISO-LWS: of NGC 1
Page 7 and 8: The 557GHz ortho-H2O line SWAS obs
Page 9 and 10: Comparison with other CO lines (CSO
Page 11 and 12: Shock chemistry: models Complex va
Page 13: Shock chemistry and internal struct

Line emission in shocks and PDR - Observatoire de Paris

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