Published 1990
| Version public
Book Section - Chapter
CO(2→1) / CO(1→0) observations of luminous infrared galaxies
Contributors
Others:
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
Identifiers
- Eprint ID
- 108104
- Resolver ID
- CaltechAUTHORS:20210217-195625533
Funding
- NSF
- AST 83-11849
Dates
- Created
-
2021-05-24Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
Caltech Custom Metadata
- Series Name
- Astrophysics and Space Science Library
- Series Volume or Issue Number
- 158