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A Hydrodynamical Model of Kepler’s Supernova Remnant Constrained by X-ray Spectra

Published online by Cambridge University Press:  12 April 2016

J. Ballet ,
M. Arnaud ,
J.P. Chieze ,
B. Magne  and
R. Rothenflug
J. Ballet
Affiliation:
–Service d’astrophysique, CEN Saclay, 91191 GIF SUR YVETTE CEDEX, FRANCE
M. Arnaud
Affiliation:
–Service d’astrophysique, CEN Saclay, 91191 GIF SUR YVETTE CEDEX, FRANCE
J.P. Chieze
Affiliation:
–Centre d’etudes de Bruyeres le Chatel, BP 12, 91680 BRUYERES LE CHATEL, FRANCE
B. Magne
Affiliation:
–Centre d’etudes de Limeil Valenton, BP 27, 94190 VILLENEUVE ST GEORGES, FRANCE
R. Rothenflug
Affiliation:
–Service d’astrophysique, CEN Saclay, 91191 GIF SUR YVETTE CEDEX, FRANCE

Abstract

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We present NEI hydrodynamical models of Kepler’s SNR compared with the EXOSAT and EINSTEIN X-ray spectra.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 141 - 144
Copyright
Copyright © Cambridge University Press 1988

References

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