Published 1990
| public
Book Section - Chapter
CO(2→1) / CO(1→0) observations of luminous infrared galaxies
Abstract
CO(2→1) spectra of several luminous infrared galaxies have been obtained with the Caltech Submillimeter Observatory (CSO). For those galaxies distant enough to be unresolved with the CSO beam, we have compared the CO(2→1) profile with the corresponding, unresolved CO(1→0) profile in order to investigate the contribution of optically thin CO to the total CO emission.
Additional Information
© Springer Science+Business Media Dordrecht 1990. The CSO is supported by NSF grant #AST 83-11849.Additional details
- Eprint ID
- 108104
- Resolver ID
- CaltechAUTHORS:20210217-195625533
- AST 83-11849
- NSF
- Created
-
2021-05-24Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Series Name
- Astrophysics and Space Science Library
- Series Volume or Issue Number
- 158