The Excited and Exciting ISM in Galaxies: PDRs, XDRs ... - Caltech

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Aykutalp & Spaans 2011
This allows one to generate atomic <strong>and</strong> molecular l<strong>in</strong>e maps at ALMA resolution (Pérez- Beaupuits ea 01).
Page 1 and 2: The Excited and Exciting ISM in Gal
Page 3 and 4: PDRs: 6 < E < 13.6 eV Heating: Phot
Page 5 and 6: Energetics G0 = 1.6x10 -3 erg cm -2
Page 8 and 9: Fine-structure lines (Kaufman et al
Page 10 and 11: Comment on AGN: Relative Size PDR/X
Page 15 and 16: [CII] 158 µm only for z>1 of cours
Page 17 and 18: Hocuk & Spaans 2010
Page 19 and 20: The Initial Mass Function Without X
Page 21 and 22: H 2 dominates for Z
Page 23 and 24: BUT: CRs ≠ X-rays; only very high
Page 25 and 26: How about shocks? M82, shock tracer
Page 27 and 28: J-shock chemistry
Page 29 and 30: HerCULES Herschel Comprehensive ULI
Page 31 and 32: Markarian 231 25 lines: 9x CO (5-4
Page 37 and 38: NGC 6240 (Meijerink ea 13)
Page 39 and 40: Shocks drive high-J CO excitation H

The Excited and Exciting ISM in Galaxies: PDRs, XDRs ... - Caltech

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