Supernova 2012aw - a high-energy clone of archetypal Type IIP SN 1999em

We present densely sampled UBVRI/griz photometric and low-resolution (6-10 Å) optical spectroscopic observations from 4 to 270 d after explosion of a newly discovered Type II SN 2012aw in a nearby (∼9.9 Mpc) galaxy M95. The light-curve characteristics of apparent magnitudes, colours, bolometric lumi...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-08, Vol.433 (3), p.1871-1891
Hauptverfasser:	Bose, Subhash, Kumar, Brijesh, Sutaria, Firoza, Kumar, Brajesh, Roy, Rupak, Bhatt, V. K, Pandey, S. B, Chandola, H. C, Sagar, Ram, Misra, Kuntal, Chakraborti, Sayan
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Fluid mechanics Luminosity Radiation Simulation Star & galaxy formation
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