STAR FORMATION IN THE RHO OPHIUCHI DARK CLOUD
New and sensitive millimeter-wave and near-infrared observation have been performed in the central regions of the ρ Ophiuchi dark cloud. High spatial resolution observations of the optically thin C¹⁸O emission lines are shown to be free of self-absorption. They permit the first accurate determinatio...
| Main Author: | |
|---|---|
| Other Authors: | |
| Language: | en_US |
| Published: |
The University of Arizona.
1981
|
| Subjects: | |
| Online Access: | http://hdl.handle.net/10150/282023 |