The compact radio source near G347.7-0.1

Details The compact radio source near G347.7-0.1 The compact radio source near G347.7-0.1

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...147l..23s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 147, no. 1, June 1985, p. L23, L24.

Astronomy and Astrophysics

Astronomy

19

Infrared Astronomy, Radio Sources (Astronomy), Supernova Remnants, Astronomical Catalogs, H Ii Regions, Spectral Energy Distribution

Scientific paper

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.

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