CO Observations of the Expanding Envelope of IRC+10216 (8),
Abstract
The authors report high-sensitivity emission profiles from the J = 0-1 transitions of (12C16O) and (13C16O) towards IRC+10216. It appears that the spherically symmetric uniform mass-outflow model proposed by Morris (1975) is necessary to describe the line profiles. The outflow appears to be slightly accelerated, having a velocity of 15 km/sec at the edges of the CO cloud, compared with 12 km/sec for the more centrally confined molecules.
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1975
- Accession Number
- ADA011098
Entities
People
- G. R. Knapp
- Robert L. Brown
- S. L. Knapp
- T. B. H. Kuiper
Organizations
- Owens Valley Radio Observatory