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VLA Observations of SNRs in M33

Published online by Cambridge University Press:  12 April 2016

N. Duric
N. Duric*
Affiliation:
Institute for Astrophysics, Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, U.S.A.

Abstract

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The results of a VLA study of the radio continuum properties of supernova remnants in the nearby spiral galaxy M33 are presented. It is shown that a relationship exists between the radio surface brightnesses and the diameters of the 13 detected supernova remnants. The significance of the relation and the constraints it imposes on models of SNR evolution are discussed.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 289 - 292
Copyright
Copyright © Cambridge University Press 1988

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