A giant outburst two years before the core-collapse of a massive star

Details A giant outburst two years before the core-collapse of a massive star A giant outburst two years before the core-collapse of a massive star

2007-03-27

arxiv.org/abs/astro-ph/0703663v2

Nature447:829-832,2007

Astronomy and Astrophysics

Astrophysics

15 pages, 4 figures (supplementary information included). Originally submitted on Nov. 24, 2006; twice revised. Final version

Scientific paper

10.1038/nature05825

The death of massive stars produces a variety of supernovae, which are linked to the structure of the exploding stars. The detection of several precursor stars of Type II supernovae have been reported, however we do not yet have direct information on the progenitors of the hydrogen deficient Type Ib and Ic supernovae. Here we report that the peculiar Type Ib supernova SN2006jc is spatially coincident with a bright optical transient that occurred in 2004. Spectroscopic and photometric monitoring of the supernova leads us to suggest that the progenitor was a carbon-oxygen Wolf-Rayet star embedded within a helium-rich circumstellar medium. There are different possible explanations for this pre-explosion transient. It appears similar to the giant outbursts of Luminous Blue Variables (LBV) of 60-100 solar mass stars, however the progenitor of SN2006jc was helium and hydrogen deficient. An LBV-like outburst of a Wolf-Rayet star could be invoked, but this would be the first observational evidence of such a phenomenon. Alternatively a massive binary system composed of an LBV which erupted in 2004, and a Wolf-Rayet star exploding as SN2006jc, could explain the observations.

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