Abstract
The author presents a far-infrared and submillimeter study of regions
within 0.03 pc of the low-luminosity sources embedded in the clouds
B335, L723, B361, L1455, and L1551. He also presents CO molecular line
results on the extended environments of these sources out to 0.3 pc.
Three of the embedded objects are definite bipolar outflow sources, one
may be associated with an observed outflow, and one has no observable
outflow. The author combines data on the outflows with the determination
of the luminosity of the embedded objects, and of the temperature and
matter distribution about the sources, to infer the evolutionary stage
of the embedded sources.
| Original language | English |
|---|---|
| Pages (from-to) | 602-620 |
| Journal | The Astrophysical Journal |
| Volume | 315 |
| DOIs | |
| Publication status | Published - 1 Apr 1987 |
| Externally published | Yes |