Photometric investigation of bright type II-P Supernova 2004dj

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CCD UBVRI photometry is presented for type II SN 2004dj for about 1200 days, starting day 2 past discovery. The photometric behaviour is typical for SNe II-P, although some minor peculiarities are noticed. We compare the photometric data for the host cluster S96 before and after SN 2004dj outburst and do not find any significant changes.
12 pages, 6 figures, submitted to Variable Stars (Peremennye Zvezdy)

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/221853

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0810.3988
 http://arxiv.org/abs/0810.3988
 Variable Stars (Peremennye Zvezdy) Vol. 28, No. 8, 2008, http://www.astronet.ru/db/varstars/msg/1231959

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arXiv