Publication Date:
2013-04-03
Description:
We present the low-resolution spectroscopic and UBVRI broad-band photometric investigations of the Type IIb supernova (SN) 2011fu, discovered in UGC 01626. The photometric follow-up of this event was initiated a few days after the explosion and covers a period of about 175 d. The early-phase light curve shows a rise, followed by steep decay in all bands, and shares properties very similar to that seen for SN 1993J, with a possible detection of the adiabatic cooling phase. Modelling of the quasi-bolometric light curve suggests that the progenitor had an extended (~1 x 10 13 cm), low-mass (~0.1 M ) H-rich envelope on top of a dense, compact (~2 x 10 11 cm), more massive (~1.1 M ) He-rich core. The nickel mass synthesized during the explosion was found to be ~0.21 M , slightly larger than that seen for other Type IIb SNe. The spectral modelling performed with synow suggests that the early-phase line velocities for H and Fe ii features were ~16 000 and ~14 000 km s –1 , respectively. Then, the velocities declined up to day +40 and became nearly constant at later epochs.
Print ISSN:
0035-8711
Electronic ISSN:
1365-2966
Topics:
Physics
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