V382 Vel: a "shocking" supersoft x-ray source?

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dc.creatorOrio, Marina
dc.creatorParmar, Arvind
dc.date2001-02-26
dc.date.accessioned2026-07-07T01:57:49Z
dc.date.available2026-07-07T01:57:49Z
dc.descriptionNova Vel 1999 (V382 Vel) was observed with BeppoSAX twice, 15 days and 6 months after the optical maximum. A hard X-ray source was detected in the first observation, while the second time also a very luminous supersoft X-ray source was detected. The continuum observed in the supersoft range with the BeppoSAX LECS cannot be fitted with atmospheric models of hot hydrogen burning while dwarfs. We suggest that we are observing instead mainly a ``pseudocontinuum'', namely a blend of very strong emission lines in the supersoft X-ray range.
dc.description1 tex file, 2 figures as .ps, a newpasp.sty file
dc.identifierhttps://arxiv.org/abs/astro-ph/0102440
dc.identifierhttp://arxiv.org/abs/astro-ph/0102440
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2535
dc.subjectAstrophysics
dc.titleV382 Vel: a "shocking" supersoft x-ray source?
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