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25 April 2024
 
  » arxiv » 1302.2633

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An outburst from a massive star 40 days before a supernova explosion
E. O. Ofek ; M. Sullivan ; S. B. Cenko ; M. M. Kasliwal ; A. Gal-Yam ; S. R. Kulkarni ; I. Arcavi ; L. Bildsten ; J. S. Bloom ; A. Horesh ; D. A. Howell ; A. V. Filippenko ; R. Laher ; D. Murray ; E. Nakar ; P. E. Nugent ; J. M. Silverman ; N. J. Shaviv ; J. Surace ; O. Yaron ;
Date 11 Feb 2013
AbstractVarious lines of evidence suggest that very massive stars experience extreme mass-loss episodes shortly before they explode as a supernova. Interestingly, several models predict such pre-explosion outbursts. Establishing a causal connection between these mass-loss episodes and the final supernova explosion will provide a novel way to study pre-supernova massive-star evolution. Here we report on observations of a remarkable mass-loss event detected 40 days prior to the explosion of the Type IIn supernova SN 2010mc (PTF 10tel). Our photometric and spectroscopic data suggest that this event is a result of an energetic outburst, radiating at least 6x10^47 erg of energy, and releasing about 0.01 Solar mass at typical velocities of 2000 km/s. We show that the temporal proximity of the mass-loss outburst and the supernova explosion implies a causal connection between them. Moreover, we find that the outburst luminosity and velocity are consistent with the predictions of the wave-driven pulsation model and disfavor alternative suggestions.
Source arXiv, 1302.2633
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