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Evolution of the Type IIb SN 2011fu
2013
Proceedings of the International Astronomical Union
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The UBVRI photometric follow-up of SN 2011fu has been initiated a few days after the explosion, shows a rise followed by steep decay in all bands and shares properties very similar to that seen in case of SN 1993J, with a possible detection of the adiabatic cooling phase at very early epochs. The spectral modeling performed with SYNOW suggests that the early-phase line velocities for H and Fe ii features were ∼ 16000 km s −1 and ∼ 14000 km s −1 , respectively. Studies of rare class of type IIb
doi:10.1017/s1743921313009708
fatcat:huixs7vflramzezeavy4f4nfre