Characterizing the Molecular Interstellar Medium in ... - Caltech
Characterizing the Molecular Interstellar Medium in ... - Caltech
Characterizing the Molecular Interstellar Medium in ... - Caltech
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Flux (Jy)<br />
600<br />
400<br />
200<br />
0<br />
CO (43)<br />
CI (10)<br />
CO (54)<br />
CO (65)<br />
M82 (Starburst)<br />
CO (76)<br />
CI (21)<br />
CO (87)<br />
CO (98)<br />
600 800 1000 1200 1400 1600<br />
rest (GHz) [used z = 0.0008]<br />
This survey will focus only on CO, CI and NII l<strong>in</strong>es. CO and CI for<br />
characteriz<strong>in</strong>g molecular gas and NII as a star formation tracer<br />
CO (109)<br />
CO (1110)<br />
CO (1211)<br />
NII 205<br />
CO (1312)<br />
CO (1413)