Photometric investigation of bright type II-P Supernova 2004dj

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dc.creatorTsvetkov, D. Yu.
dc.creatorGoranskiy, V. P.
dc.creatorPavlyuk, N. N.
dc.date2008-10-22
dc.date2008-10-23
dc.date.accessioned2026-07-07T12:47:50Z
dc.date.available2026-07-07T12:47:50Z
dc.descriptionCCD 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.
dc.description12 pages, 6 figures, submitted to Variable Stars (Peremennye Zvezdy)
dc.identifierhttps://arxiv.org/abs/0810.3988
dc.identifierhttp://arxiv.org/abs/0810.3988
dc.identifierVariable Stars (Peremennye Zvezdy) Vol. 28, No. 8, 2008, http://www.astronet.ru/db/varstars/msg/1231959
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/221853
dc.subjectAstrophysics
dc.titlePhotometric investigation of bright type II-P Supernova 2004dj
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