The arrival of a shock wave at the surface of a compact presupernova and SN 1987A in the Large Magellanic Cloud

Details The arrival of a shock wave at the surface of a compact presupernova and SN 1987A in the Large Magellanic Cloud The arrival of a shock wave at the surface of a compact presupernova and SN 1987A in the Large Magellanic Cloud

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14.1059i&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Dec. 1988, p. 1059-1065. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

3

Magellanic Clouds, Shock Wave Propagation, Supernova 1987A, Ultraviolet Astronomy, X Ray Astronomy, Propagation Velocity, Stellar Envelopes, Stellar Temperature

Scientific paper

The emergence of a shock wave from the surface of a massive compact star
is shown to result in a short pulse of a soft X-ray and hard ultraviolet
radiation of total energy about ≡1047ergs. Numerical
evaluations of maximum temperature and velocity acquired by outermost
layers of the star in the case of SN 1987A are presented.

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