Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-02-14
Peremennye Zvezdy (Variable Stars), 2008, vol. 28, N 3, http://www.astronet.ru/db/varstars/msg/1226985
Astronomy and Astrophysics
Astrophysics
4 pages, 7 figures, 3 tables, submitted to Variable Stars
Scientific paper
CCD BVRI photometry is presented for type II Supernovae 2004A and 2004ek. SN 2004A is found to be a typical SN II-P, with the shape of the light and color curves and maximum luminosity closely matching those for SN 1999em. SN 2004ek shows unusual light curves with long flat plateau in the B band, two peaks in the V and prominent brightening in the R and I bands, starting about 45 days past outburst. The brightness decline after the plateau stage is probably quite slow. The plateau luminosity is about 1.5 mag brighter than average for SN II-P.
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