The compact radio source near G 357.7-0.1.
Abstract
Since the compact source near the SNR G357.7-0.1 is probably a normal H II region, it is held to be an unlikely site for an accreting binary system powering G357.7-0.1, as suggested by Helfand and Becker (1985). It may instead be a line-of-sight object totally unassociated with the SNR, or the two objects could be located in the same OB association. It is suggested that G357.7-0.1's unusual morphology may be due to the occurrence of a supernova explosion near the edge of a molecular cloud containing the H II region.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- June 1985
- Bibcode:
- 1985A&A...147L..23S
- Keywords:
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- Infrared Astronomy;
- Radio Sources (Astronomy);
- Supernova Remnants;
- Astronomical Catalogs;
- H Ii Regions;
- Spectral Energy Distribution;
- Astronomy