Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S296(9), p. 112-115, 2013
DOI: 10.1017/s1743921313009320
Full text: Unavailable
AbstractSN 2012AW is a type-IIP supernova which exploded in M95. In this paper we discuss the radio observations of this supernova and model them to determine the important parameters relevant to the explosion and the evolution of blast wave. We also determine the dominant cooling process important to this source.