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.
@article{arxiv.0810.3988,
title = {Photometric investigation of bright type II-P Supernova 2004dj},
author = {D. Yu. Tsvetkov and V. P. Goranskiy and N. N. Pavlyuk},
journal= {arXiv preprint arXiv:0810.3988},
year = {2009}
}
Comments
12 pages, 6 figures, submitted to Variable Stars (Peremennye Zvezdy)