The late UVOIR light curve of SN 2000cx

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dc.creatorSollerman, Jesper
dc.creatorKozma, Cecilia
dc.creatorLindahl, Jan
dc.date2003-11-04
dc.date.accessioned2026-07-07T02:11:03Z
dc.date.available2026-07-07T02:11:03Z
dc.descriptionWe present preliminary data and modeling of the late time light curve of the Type Ia supernova SN 2000cx. Optical and near-infrared data obtained with the VLT at 360 to 480 days past maximum light show the increasing importance of the near-infrared regime. Detailed multi-band modeling based on W7 also show this effect. Conclusions on positron escape in this phase may therefore require more detailed observations and modeling than hitherto appreciated.
dc.descriptionTo appear in proceedings of IAU Colloquium 192, Supernovae: 10 Years of 1993J, Valencia, Spain 22-26 April 2003, eds. J.M. Marcaide, K.W. Weiler
dc.identifierhttps://arxiv.org/abs/astro-ph/0311075
dc.identifierhttp://arxiv.org/abs/astro-ph/0311075
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6944
dc.subjectAstrophysics
dc.titleThe late UVOIR light curve of SN 2000cx
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