SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared

Details SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared

2009-01-14

arxiv.org/abs/0901.2075v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

18 pages, 18 figures, accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2009.14505.x

We present the results of the one year long observational campaign of the type II-plateau SN 2005cs, which exploded in the nearby spiral galaxy M51 (the Whirlpool Galaxy). This extensive dataset makes SN 2005cs the best observed low-luminosity, 56Ni-poor type II-plateau event so far and one of the best core-collapse supernovae ever. The optical and near-infrared spectra show narrow P-Cygni lines characteristic of this SN family, which are indicative of a very low expansion velocity (about 1000 km/s) of the ejected material. The optical light curves cover both the plateau phase and the late-time radioactive tail, until about 380 days after core-collapse. Numerous unfiltered observations obtained by amateur astronomers give us the rare opportunity to monitor the fast rise to maximum light, lasting about 2 days. In addition to optical observations, we also present near-infrared light curves that (together with already published UV observations) allow us to construct for the first time a reliable bolometric light curve for an object of this class. Finally, comparing the observed data with those derived from a semi-analytic model, we infer for SN 2005cs a 56Ni mass of about 0.003 solar masses, a total ejected mass of 8-13 solar masses and an explosion energy of about 3 x 10^50 erg.

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