No CrossRef data available.
Article contents
The X-ray Emission from SN 1987A and the Remnant of SN 1572 (Tycho)
Published online by Cambridge University Press: 12 April 2016
Abstract
The thermal X-ray emission from SN 1987A may be enhanced to a detectable level when the blast shock hits the circumstellar medium which has formed in the red-supergiant stage of the progenitor.
The X-ray spectrum of Tycho observed with the satellite Tenma can be explained approximately within the context of a carbon deflagration model for Type la supernovae, if the ejecta are assumed to be mixed partially.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 149 - 152
- Copyright
- Copyright © Cambridge University Press 1988