The soft X-ray background as a supernova blast wave viewed from inside - Solar abundance models
A model of the soft X-ray background is presented in which the sun is assumed to be inside an active supernova blast wave. The blast wave evolves in a preexisting cavity. The broad band surface brightnesses is explained by such a blast wave with an explosion energy of E sub approximately 5 x 10 to t...
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Veröffentlicht in: | The Astrophysical journal 1986-09, Vol.308 (1), p.389-400 |
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Format: | Artikel |
Sprache: | eng |
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