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A Theoretical Model of the Cygnus Loop and its X-ray Emission

Published online by Cambridge University Press:  04 August 2017

S. A. E. G. Falle  and
A. R. Garlick
S. A. E. G. Falle
Affiliation:
Department of Applied Mathematics University of Leeds, Leeds, England
A. R. Garlick
Affiliation:
Department of Applied Mathematics University of Leeds, Leeds, England

Abstract

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In this paper we present a theoretical model of the Cygnus Loop which, with only a small number of free parameters, accounts for most of the gross features of the observations. We believe that none of the models described in the literature can explain the observations in such a simple way.

Type
II. Middle Aged and Older Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 261 - 266
Copyright
Copyright © Reidel 1983 

References

De Noyer, L.K. 1975, Astrophys. J., 196, 479.Google Scholar
Falle, S.A.E.G. 1981, Mon. Not. R. astr. Soc., 195, 1011.Google Scholar
Hubble, E.P. 1937, Carnegie Yrb., No. 36, p. 189.Google Scholar
Kirschner, R.P. and Taylor, K. 1976, Astrophys. J., 208, L83.CrossRefGoogle Scholar
Laan, H. van der, 1962, Mon. Not. R. astr. Soc., 124, 127.Google Scholar
Miller, J.S. 1974, Astrophys. J., 189, 239.Google Scholar
Minkowski, R. 1958, Rev. Mod. Phys., 30, 1048.CrossRefGoogle Scholar
Moffat, P.H. 1971, Mon. Not. R. astr. Soc., 153, 401.Google Scholar
Rappaport, S., Doxsey, R., Solinger, A., and Borken, R. 1974, Astrophys. J., 194, 329.Google Scholar
Rappaport, S., Petre, R., Kayat, M.A., Evans, K.D., Smith, G.C., and Levine, A. 1979, Astrophys. J., 227, 285.Google Scholar