Light Curve Models of Supernovae and X-ray spectra of Supernova Remnants

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dc.creatorBlinnikov, S. I.
dc.creatorBaklanov, P. V.
dc.creatorKozyreva, A. V.
dc.creatorSorokina, E. I.
dc.date2004-09-16
dc.date.accessioned2026-07-07T02:14:38Z
dc.date.available2026-07-07T02:14:38Z
dc.descriptionWe compare parameters of well-observed type II SN1999em derived by M.Hamuy and D.Nadyozhin based on Litvinova-Nadyozhin (1985) analytic fits with those found from the simulations with our radiative hydro code Stella. The difference of SN parameters is quite large for the long distance scale. The same code applied to models of SN1993J allows us to estimate systematic errors of extracting foreground extinction toward SN1993J suggested by Clocchiatti et al. (1995). A new implicit two-temperature hydro code code Supremna is introduced which self-consistently takes into account the kinetics of ionization, electron thermal conduction, and radiative losses for predicting X-ray spectra of young supernova remnants such as Tycho and Kepler.
dc.description7 pages, 10 figures, Supernovae as Cosmological Lighthouses, Padua, June 16- 19, 2004, eds. M.Turatto et al., ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0409396
dc.identifierhttp://arxiv.org/abs/astro-ph/0409396
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8194
dc.subjectAstrophysics
dc.titleLight Curve Models of Supernovae and X-ray spectra of Supernova Remnants
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