Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6559
Title: Evolution of the Type IIb SN 2011fu
Authors: Pandey, S. B
Kumar, B
Sahu, D. K
Vinko, J
Moskvitin, A. S
Anupama, G. C
Bhatt, V. K
Ordasi, A
Nagy, A
Sokolov, V. V
Sokolova, T. N
Komarova, V. N
Kumar, B
Bose, S
Roy, R
Sagar, R
Keywords: Supernovae: general;supernovae: individual (SN2011fu)
Issue Date: Jan-2014
Publisher: Cambridge University Press
Citation: Proceedings of the International Astronomical Union, Vol. 296, pp. 336-337
Series/Report no.: International Astronomical Union Symposium;296
Abstract: 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 SNe are important to understand the evolution of the possible progenitors of core-collapse SNe in more details.
Description: Restricted Access
URI: http://hdl.handle.net/2248/6559
ISBN: 978-1-107-04477-7
ISSN: 1743-9213
???metadata.dc.rights???: © International Astronomical Union
???metadata.dc.relation.uri???: http://dx.doi.org/10.1017/S1743921313009708
Appears in Collections:IIAP Publications

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