Characterizing the Molecular Interstellar Medium in ... - Caltech

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CO SLEDs Normalized Luminosity 10 7 10 6 0 115 230 345 461 576 691 806 922 1037 1152 1267 1382 1497 1611 Mrk 231 (AGN) UGC05101 (AGN) Arp 220 (ULIRG/starburst) M82 (starburst) NGC7552 (barred spiral) Milky Way Frequency (GHz) 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 Jupper Using a large sample we will establish if the shape and brightness of the CO SLED in galaxies can be used as a diagnostic between dominant sources of energy affecting their molecular ISM and star formation.
Dust Modeling Arp220 NGC 6240 S( )= Nbb(1 e 0 e hc kT 1 )(c/ ) 3 + Npl ↵ e ( / c) 2
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 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: 3 4 5 6 Log 10 n(H 2) (cm 3 ) 4 5 6
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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