Abstract
Submillimetre HCO+(J = 4 − 3) mapping observations of the immediate environs of the infrared source IRS 7 in Corona Australis have provided corroborative evidence for the existence of the rotating molecular disk detailed in our earlier paper. An improved estimate of 0.8M ¯ for the mass of the central protostar is obtained. Accepted by A & A
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Publication Info
- Year
- 1997
- Type
- article
- Volume
- 288
- Issue
- 4
- Pages
- 1060-1072
- Citations
- 513
- Access
- Closed
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Identifiers
- DOI
- 10.1093/mnras/288.4.1060