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arXiv · 0810.3988

Photometric investigation of bright type II-P Supernova 2004dj

D. Yu. Tsvetkov·V. P. Goranskiy·N. N. Pavlyuk
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Abstract

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.

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D. Yu. Tsvetkov, V. P. Goranskiy, N. N. Pavlyuk. 2008-10-23. Photometric investigation of bright type II-P Supernova 2004dj. https://arxiv.org/abs/0810.3988

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