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|Title: ||Far-Infrared Spectroscopy of M82: Interstellar Properties of the Dual Nuclear Starbursts|
|Authors: ||Lord, S. D.|
Hollenbach, D. J.
Haas, M. R.
Rubin, R. H.
Colgan, S. W. J.
Erickson, E. F.
|Issue Date: ||1995 |
|Citation: ||The Astrophysical Journal|
|Abstract: ||We have measured [O I] 63 mm and [Si II] 35 mm in the central 44" (700 pc) of the starburst galaxy M82. The luminosities in these transitions are each ~0.1 percent of the bolometric luminosity. We model the [O I] in M82 as arising from warm neutral gas photodissociated by FUV flux from OB stars, while most of the [Si II] emission arises from associated H II regions.!|
|Appears in Collections:||JPL TRS 1992+|
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