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Title:
Radio and X-ray observations of G11.2 - 0.3 and G41.1 - 0.3
Authors:
Becker, R. H.; Markert, T.; Donahue, M.
Affiliation:
AA(California, University, Davis), AB(MIT, Cambridge, MA), AC(MIT, Cambridge, MA)
Publication:
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 296, Sept. 15, 1985, p. 461-468. (ApJ Homepage)
Publication Date:
09/1985
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
ASTRONOMICAL SPECTROSCOPY, RADIO SOURCES (ASTRONOMY), SUPERNOVA REMNANTS, X RAY SOURCES, BRIGHTNESS, MORPHOLOGY, NEBULAE
DOI:
10.1086/163465
Bibliographic Code:
1985ApJ...296..461B

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.

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