Characterizing the Molecular Interstellar Medium in ... - Caltech

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Flux [Jy] • • 50 40 30 20 10 CO (43) CI (10) CH CH CO (54) CO (65) HCN 87 HCO+ 87 H2O + H2O + H2O 211202 HCN 98 HCO+ 98 CO (76) CI (21) CH + HCN 109 HCO+ 109 NH2 OH + CO (87) NH2 OH + HCN 1110 NH HCO+ 1110 H2O 202111 NH OH + CO (98) HCN 1211 HCO+ 1211 H2O 312303 H2O 111000 H2O + H2O + HCN 1312 CO (109) H2O 312221 HCO+ 1312 H2O 321312 H2O 422413 NH3 H2O 220211 HF HCN 1413 HCO+ 1413 CO (1110) HCN 1514 HCO+ 1514 CO (1211) H2O 523514 HCN 1615 HCO+ 1615 NH2 NH2 NII CH CH CO (1312) HCN 1716 HCO+ 1716 0 670 µm SPIRE-FTS spectrum of Arp 220 300 µm 600 800 1000 rest [GHz] 1200 1400 Continuous spectral coverage spectral resolution = 1.44 GHz • • Rangwala et al. (2011) several molecular and atomic species 190 µm CO rotational transitions from J = 4-3 to 13-12
• • Description of our Archival Program Archival (publicly available) survey using photometric and spectroscopic data of all the galaxies (~300) observed with Herschel- SPIRE’s Fourier Transform Spectrometer (FTS). This sample spans a wide range in the far-infrared luminosity (L FIR) and galaxy types.
Page 1 and 2: Characterizing the Molecular Inters
Page 3: • Description of our Archival Pro
Page 7 and 8: • • • • Description of our
Page 9 and 10: Normalized Luminosity 10 7 10 6 CO
Page 11 and 12: Herschel! Archive! Literature! data
Page 13 and 14: Flux (Jy) 600 400 200 0 CO (43) CI
Page 15 and 16: Flux (Jy) 10 8 6 4 2 0 CO (43) CI (
Page 17 and 18: Modeling and Preliminary Results
Page 19 and 20: Arp 220: Excitation source of warm
Page 21 and 22: 3 4 5 6 Log 10 n(H 2) (cm 3 ) 4 5 6
Page 23 and 24: Dust Modeling Arp220 NGC 6240 S( )=
Page 25 and 26: Extra Slides
Page 27 and 28: UGC 05101 (LIRG/AGN) Flux [Jy] 3456
Page 29 and 30: L CO (65) (L sun) 10 10 10 9 10 8 1
Page 31 and 32: 3060 M. S. Bothwell et al. 4.3 The

Characterizing the Molecular Interstellar Medium in ... - Caltech

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