Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-03-27
Peremennye Zvezdy (Variable Stars), 2008, vol. 28, N 6
Astronomy and Astrophysics
Astrophysics
8 pages, 5 figures, submitted to Variable Stars
Scientific paper
CCD UBVRI photometry is presented for type IIn SN 2005kd. The maximum
luminosity exceeded Mv=-19.8, and SN remained brighter than -18 mag for about
400 days. While overall photometric evolution is quite similar to SN 1997cy, SN
2005kd shows a plateau at phases between 119 and 311 days past explosion, which
is a unique feature for SN IIn.
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