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Modeling the X-Rays from SNe 1993J & 1998S
Stockholm University.
(Stockholm University)
2007 (English)In: Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters / [ed] Immler, S; Weiler, K; McCray, R, American Institute of Physics (AIP), 2007, Vol. 937, 430-432 p.Conference paper, Published paper (Refereed)
Abstract [en]

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 Xray 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 shocks while the X-ray flux for SN 1993J is dominated by the reverse shock.

Place, publisher, year, edition, pages
American Institute of Physics (AIP), 2007. Vol. 937, 430-432 p.
Series
American Institute of Physics Conference Series, ISSN 0094-243X ; 937
Keyword [en]
Supernovae, X-ray, Circumstellar shells, clouds, and expanding envelopes; circumstellar masers
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-86984DOI: 10.1063/1.2803603ISI: 000251154500064ISBN: 978-0-7354-0448-9 (print)OAI: oai:DiVA.org:kth-86984DiVA: diva2:502893
Conference
SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters; Aspen, CO; 19 February 2007 through 23 February 2007
Note
QC 20120217Available from: 2012-02-14 Created: 2012-02-14 Last updated: 2012-02-17Bibliographically approved

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CiteExportLink to record
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Citation style
  • apa
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  • nn-NB
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  • Other locale
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