Photometric investigation of bright type II-P Supernova 2004dj
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🌌 astro-ph
keywords
photometricii-ptypealthoughbeforebehaviourbrightchanges
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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.
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