The Search for Failed Supernovae with The Large Binocular Telescope: First Candidates
Nov 6, 201417 pages
Published in:
- Mon.Not.Roy.Astron.Soc. 450 (2015) 3, 3289-3305
- Published: Jul 1, 2015
e-Print:
- 1411.1761 [astro-ph.SR]
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Abstract: (Oxford University Press)
We are monitoring 27 galaxies within 10 Mpc using the Large Binocular Telescope to search for failed supernovae (SNe), massive stars that collapse to form a black hole without an SN explosion. We present the results from the first 4 yr of survey data, during which these galaxies were observed to produce three successful core-collapse SNe. We search for stars that have ‘vanished’ over the course of our survey, by examining all stars showing a decrease in luminosity of ΔνL_ν ≥ 10^4 L_⊙ from the first to the last observation. We also search for the low luminosity, long duration transients predicted by Lovegrove & Woosley (2013) for failed explosions of red supergiants. After analysing the first 4 yr of data in this first direct search for failed SNe, we are left with one candidate requiring further study. This candidate has an estimated mass of 18–25 M_⊙, a mass range likely associated with failed SNe and, if real, implies that failed SN represents a median fraction of f ≃ 0.30 of core collapses, with symmetric 90 per cent confidence limits of 0.07 ≤ f ≤ 0.62. If follow up data eliminate this candidate, we find an upper limit on the fraction of core collapses leading to a failed SN of f < 0.40 at 90 per cent confidence. As the duration of the survey continues to increase, it will begin to constrain the f ≃ 10–30 per cent failure rates needed to explain the deficit of massive SN progenitors and the observed black hole mass function.Note:
- Submitted to MNRAS. 19 pages, 16 figures. For a brief video abstract of the paper, please visit https://www.youtube.com/watch?v=9C-PIspuKJk&list=UU0YbHd6wHHz98SUJYGAXcUA
- black hole physics
- surveys
- stars: massive
- supernovae: general
References(108)
Figures(16)