Interstellar Carbon Monosulfide
Abstract
We have observed line emission from the 146969.16-MHz j = 3 to j = 2 transition in CS in four sources. Typical column densities are near 1014 molecules cm . The excitation rates required to produce the observed line intensities are used to derive densities for the central regions of the sources.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- September 1971
- DOI:
- 10.1086/180784
- Bibcode:
- 1971ApJ...168L..53P