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

More documents

Recommendations

Info

Mrk 231; SPIRE, IR pumping of water lines by dust emission (González-Alfonso ea 10) APM 08279+5255 Lensed QSO (3 images); SMBH 10 9.5 M o z=3.9; water ~ dust ~ 220 K Lensing magnification µ = 4 (van der Werf ea 11)
HerCULES Herschel Comprehensive ULIRG Emission Survey (PI: van der Werf) Measure gas cooling lines in a flux-limited sample of 29 (U)LIRGs; high-z template Observations: High resolution SPIRE FTS: CO, [CI], [NII], etc. PACS: [CII] 158µm, [OI] 63 and 146 µm All targets observed to same (expected) S/N Extended sources observed at several positions
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 12 and 13: Aykutalp & Spaans 2011
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: J-shock chemistry
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

Create successful ePaper yourself

Delete template?

Save as template?