Radio and X-ray observations of G 11.2-0.3 and G 4.1-0.3.
Abstract
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.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- September 1985
- DOI:
- Bibcode:
- 1985ApJ...296..461B
- Keywords:
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- Astronomical Spectroscopy;
- Radio Sources (Astronomy);
- Supernova Remnants;
- X Ray Sources;
- Brightness;
- Morphology;
- Nebulae;
- Astrophysics