CCD UBVRI photometry is presented for type IIb SN 2011dh for about 300 days. The main photometric parameters are derived and the comparison with SNe of similar types is reported. The light curves are similar to those for SN IIb 2008ax, but the initial flash is stronger and very short, and there are humps on the light curves in U and B at the onset of linear decline. Preliminary modeling is carried out, and the results are compared to the quasi-bolometric light curve and to the light curves in UBVRI bands.
@article{arxiv.1207.2241,
title = {Photometric observations and preliminary modeling of type IIb supernova 2011dh},
author = {D. Yu. Tsvetkov and I. M. Volkov and E. I. Sorokina and S. I. Blinnikov and N. N. Pavlyuk and G. V. Borisov},
journal= {arXiv preprint arXiv:1207.2241},
year = {2012}
}
Comments
14 pages, 9 figures, submitted to Variable Stars (Peremennye Zvezdy)