Modeling the X-rays from SNe 1993J & 1998S

Details Modeling the X-rays from SNe 1993J & 1998S Modeling the X-rays from SNe 1993J & 1998S

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..937..430n&link_type=abstract

SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP Conference Proceedings, Volume 937, pp. 430-432 (2007).

Computer Science

Supernovae, X-Ray, Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers

Scientific paper

The X-ray emission from the Type II supernovae SNe 1993J and 1998S is modelled using the numerical code described in Nymark et al. (2006), assuming that most of the observed X-ray emission comes from the reverse shock created by the interaction between the supernova ejecta and a dense circumstellar medium. We find that the spectra of both SNe are compatible with a CNO-enriched composition. For SN 1998S we find evidence for a component from both the reverse and forward shock, while the X-ray flux for SN 1993J is dominated by the reverse shock.

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