Characterizing the Molecular Interstellar Medium in ... - Caltech

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Flux (Jy) 12 10 8 6 4 2 0 CO (43) CI (10) CO (54) NGC 6240 (LIRG/AGN) CO (65) CO (76) CI (21) CO (87) CO (98) 600 800 1000 1200 1400 1600 rest (GHz) [used z = 0.0243] CO (109) CO (1110) CO (1211) NII 205 CO (1312) CO (1413)
Flux (Jy) 10 8 6 4 2 0 CO (43) CI (10) CO (54) MRK 231 (ULIRG/AGN) CO (65) CO (76) CI (21) CO (87) CO (98) 600 800 1000 1200 1400 1600 rest (GHz) [used z = 0.0418] CO (109) CO (1110) CO (1211) NII 205 CO (1312) CO (1413)
Page 1 and 2: Characterizing the Molecular Inters
Page 3 and 4: • Description of our Archival Pro
Page 5 and 6: • • Description of our Archival
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: Flux (Jy) 600 400 200 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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