Radio and X-ray observations of G11.2 - 0.3 and G41.1 - 0.3

Details Radio and X-ray observations of G11.2 - 0.3 and G41.1 - 0.3 Radio and X-ray observations of G11.2 - 0.3 and G41.1 - 0.3

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...296..461b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 296, Sept. 15, 1985, p. 461-468.

Astronomy and Astrophysics

Astronomy

29

Astronomical Spectroscopy, Radio Sources (Astronomy), Supernova Remnants, X Ray Sources, Brightness, Morphology, Nebulae

Scientific paper

The supernova remnants G11.2 - 0.3 and G41.1 - 0.3 have been observed in radio and X-ray utilizing the VLA and Einstein Observatory, respectively. The acquired images reveal that both sources have shell morphologies and do not exhibit any clear indication of a central stellar remnant. In addition, both objects are relatively bright X-ray sources.

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