Peremennye Zvezdy ( Variable Stars ) 32 , No. ... 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 and 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. ... The light curves of SN 2011dh. The dashed lines are the light curves of SN 2008ax. ... 0.03 . ... K100a . ...