Published 1990
| public
Book Section - Chapter
A search for dense gas around young stars
Chicago
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Abstract
We searched for CS(7–6) emission in a range of young stars, to test for the presence of dense gas. CS emission was detected only towards high-luminosity objects. We suggest that this is because the low-luminosity objects cannot heat a sufficient volume of gas to produce detectable CS emission.
Additional Information
© Springer Science+Business Media Dordrecht 1990. This research was supported by NSF grant AST 83-11849.Additional details
- Eprint ID
- 106762
- Resolver ID
- CaltechAUTHORS:20201120-120817396
- NSF
- AST 83-11849
- Created
-
2020-11-23Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)
- Series Name
- Astrophysics and Space Science Library
- Series Volume or Issue Number
- 158