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The X-ray Appearance of Supernova Remnants in Tenuous Media

Authors :
Denis F. Cioffi
Source :
Symposium - International Astronomical Union. 144:355-358
Publication Year :
1991
Publisher :
Cambridge University Press (CUP), 1991.

Abstract

By estimating the X-ray intensities of old supernova remnants in the disk-halo interface, deductions can be made about the ability of isolated supernovae to have created a coronal halo.

Subjects

Subjects :
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics::Galaxy Astrophysics

Details

ISSN :
00741809
Volume :
144
Database :
OpenAIRE
Journal :
Symposium - International Astronomical Union
Accession number :
edsair.doi...........67d8c2311e0b82983f43709cd3a2d840
Full Text :
https://doi.org/10.1017/s0074180900089294
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