Photometric Observations of Supernova 2002hh
D. Yu. TsvetkovM. M. MuminovUlugh Bek Astronomical Institute of Uzbekistan Academy of SciencesO. A. BurkhanovUlugh Bek Astronomical Institute of Uzbekistan Academy of SciencesB. B. KahharovUlugh Bek Astronomical Institute of Uzbekistan Academy of Sciences
2007en
ABI
Annotatsiya
CCD VRI photometry is presented for SN 2002hh from 14 days after the outburst till day 347. SN 2002hh appears to be normal type IIP supernova regarding both luminosity and the shape of the light curve, which is similar to SN 1999gi.
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