The search for failed supernovae with the Large Binocular Telescope: a new candidate and the failed SN fraction with 11 yr of data
arXiv:2104.03318 · doi:10.1093/mnras/stab2605
Abstract
We present updated results of the Large Binocular Telescope Search for Failed Supernovae. This search monitors luminous stars in 27 nearby galaxies with a current baseline of 11~yr of data. We re-discover the failed supernova (SN) candidate N6946-BH1 as well as a new candidate, M101-OC1. M101-OC1 is a blue supergiant that rapidly disappears in optical wavelengths with no evidence for significant obscuration by warm dust. While we consider other options, a good explanation for the fading of M101-OC1 is a failed SN, but follow-up observations are needed to confirm this. Assuming only one clearly detected failed SN, we find a failed SN fraction at 90 per~cent confidence. We also report on a collection of stars that show slow (decade), large amplitude () luminosity changes.
14 pages, 11 figures, 5 tables, 2 machine-readable tables (included as ancillary txt files)
References in corpus (21)
- Binary interaction dominates the evolution of massive stars
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
- The death of massive stars - I. Observational constraints on the progenitors of type II-P supernovae
- Observational constraints on the progenitors of core-collapse supernovae : the case for missing high mass stars
- Empirical Color Transformations Between SDSS Photometry and Other Photometric Systems
- Kinematics of the Local Universe XIII. 21-cm line measurements of 452 galaxies with the Nançay radiotelescope, JHK Tully-Fisher relation and preliminary maps of the peculiar velocity field
- The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields
- A new mass-loss rate prescription for red supergiants
- The Search for Failed Supernovae with The Large Binocular Telescope: First Candidates
- Planetary Nebulae in Face-On Spiral Galaxies. I. Planetary Nebula Photometry and Distances
- A Unicorn in Monoceros: the dark companion to the bright, nearby red giant V723 Mon is a non-interacting, mass-gap black hole candidate
- The light curve of SN 1987A revisited: constraining production masses of radioactive nuclides
- Constraints on Core Collapse from the Black Hole Mass Function
- A Search for Stellar-Mass Black Holes via Astrometric Microlensing
- Supernova Progenitors, Their Variability, and the Type IIP Supernova ASASSN-16fq in M66
- Discovery of a very young high-mass X-ray binary associated with the supernova remnant MCSNRJ0513-6724 in the LMC
- Luminous Red Nova 2015 in the Galaxy M101
- On the Progenitor of the Type Ic Supernova 2012fh
- The Massive Star Population in M101. III. Spectra and Photometry of the Luminous and Variable Stars
- The Search for Failed Supernovae with the Large Binocular Telescope: N6946-BH1, Still No Star
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- Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
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- From Galactic Chemical Evolution to Cosmic Supernova Rates Synchronized with Core-Collapse Supernovae Limited to the Narrow Progenitor Mass Range
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- Discovering vanishing objects in POSS I red images using the Virtual Observatory
- Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
- The Progenitor of the Vela Pulsar
- Diffuse Neutrino Background from Magnetorotational Stellar Core Collapses
- First Detailed Calculation of Atmospheric Neutrino Foregrounds to the Diffuse Supernova Neutrino Background in Super-Kamiokande
- Disappearance of a massive star in the Andromeda Galaxy due to formation of a black hole
- A rapidly fading star as a type II obscuring intermediate luminosity optical transient (ILOT) in a triple star system
- Triangulating Black Hole Forming Stellar Collapses through Neutrinos
- Properties of Thorne-Zytkow object explosions
- Hertzsprung gap stars in nearby galaxies and the Quest for Luminous Red Novae Progenitors
- Neutrinos from Diffuse Supernova Background
- Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
- High-Energy Neutrinos from Cosmic-Ray Scatterings with Supernova Neutrinos