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Modeling the X‐rays from SNe 1993J & 1998S
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- Nymark, Tanja (author)
- Stockholms universitet,Institutionen för astronomi
- Chandra, Poonam (author)
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- Fransson, Claes (author)
- Stockholms universitet,Institutionen för astronomi
- (creator_code:org_t)
- AIP, 2007
- 2007
- English.
- In: AIP Conference Proceedings. - : AIP. - 0094-243X .- 1551-7616. - 9780735404489 ; 937:430, s. 430-432
- Journal article (peer-reviewed)
Abstract
Subject headings
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- TheX-ray emission from the Type II supernovae SNe 1993J and1998S is modelled using the numerical code described in Nymarket al. (2006), assuming that most of the observed X-ray emissioncomes from the reverse shock created by the interaction betweenthe supernova ejecta and a dense circumstellar medium. We findthat the spectra of both SNe are compatible with aCNO-enriched composition. For SN 1998S we find evidence for acomponent from both the reverse and forward shock, while theX-ray flux for SN 1993J is dominated by the reverseshock.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- supernovae
- X-ray emission spectra
- circumstellar matter
- shock waves
- Astronomy and astrophysics
- Astronomi och astrofysik
Publication and Content Type
- ref (subject category)
- art (subject category)
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