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Please use this identifier to cite or link to this item:
http://hdl.handle.net/2014/32233
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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.! |
| URI: | http://hdl.handle.net/2014/32233 |
| Appears in Collections: | JPL TRS 1992+
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