A synchrotron model for the X-ray emission from supernova 1987A

Details A synchrotron model for the X-ray emission from supernova 1987A A synchrotron model for the X-ray emission from supernova 1987A

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988natur.332..418b&link_type=abstract

Nature (ISSN 0028-0836), vol. 332, March 31, 1988, p. 418, 419.

Computer Science

22

Supernova 1987A, Synchrotron Radiation, X Ray Sources, Compton Effect, Nebulae, Pulsars, Stellar Envelopes

Scientific paper

An X-ray source coincident with supernova 1987A has recently been discovered. To model the X-ray emission, the authors propose that a synchrotron nebula has been formed by a pulsar and that the supernova envelope is fragmented. This would permit the central region to be seen directly, leading to a secular light curve on which transient obscurations are superimposed.

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