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Title:
A multiwavelength comparison of Cassiopeia A and Tycho's supernova remnant [ Erratum: 1983ApJ...264..746D ]
Authors:
Dickel, J. R.; Murray, S. S.; Morris, J.; Wells, D. C.
Affiliation:
AA(Illinois, University, Urbana, IL), AB(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA), AC(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA), AD(Kitt Peak National Observatory, Tucson, AZ)
Publication:
Astrophysical Journal, Part 1, vol. 257, June 1, 1982, p. 145-150. (ApJ Homepage)
Publication Date:
06/1982
Category:
Astronomy
Origin:
STI
NASA/STI Keywords:
CASSIOPEIA A, RADIO SOURCES (ASTRONOMY), STELLAR SPECTRA, SUPERNOVA REMNANTS, X RAY SOURCES, ASTRONOMICAL MAPS, EMISSION SPECTRA, HIGH RESOLUTION, LIGHT (VISIBLE RADIATION), SPECTRUM ANALYSIS, STELLAR EVOLUTION
Comment:
A&AA ID. AAA031.125.027
DOI:
10.1086/159972
Bibliographic Code:
1982ApJ...257..145D

Abstract

A comparison of high resolution radio, optical, and X-ray images of two young supernova remnants (SNR), Cas A and Tycho, shows significant differences between them. Cas A probably broke into many small knots at the time of the initial explosion, whereas Tycho's SNR appears to be a more uniformly expanding blast wave.

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