An enhanced rate of tidal disruptions in the centrally overdense E+A galaxy NGC 3156

Journal Article · Fri Jul 01 04:00:00 EDT 2016 · Astrophysical Journal Letters

DOI:https://doi.org/10.3847/2041-8205/825/1/L14· OSTI ID:22868935

Stone, Nicholas C. ^[1]

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1. Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027 (United States)

Time domain optical surveys have discovered roughly a dozen candidate stellar tidal disruption flares in the last five years, and future surveys like the Large Synoptic Survey Telescope will likely find hundreds to thousands more. These tidal disruption events (TDEs) present an interesting puzzle: a majority of the current TDE sample is hosted by rare post-starburst galaxies, and tens of percents of the galaxies are hosted in even rarer E+A galaxies, which make up ∼0.1% of all galaxies in the local universe. E+As are therefore overrepresented among TDE hosts by 1–2 orders of magnitude, a discrepancy unlikely to be accounted for by selection effects. We analyze Hubble Space Telescope photometry of one of the nearest E+A galaxies, NGC 3156, to estimate the rate of stellar tidal disruption produced as two-body relaxation diffuses stars onto orbits in the loss cone of the central supermassive black hole. The rate of TDEs produced by two-body relaxation in NGC 3156 is large when compared to other galaxies with similar black hole mass: N-dot {sub TDE}∼1×10{sup −3} yr{sup −1}. This suggests that the preference of TDEs for E+A hosts may be due to central stellar overdensities produced in recent starbursts.

• OSTI ID: 22868935
• Journal Information: Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 1 Vol. 825; ISSN 2041-8205
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
BLACK HOLES
DENSITY
GALAXY NUCLEI
LOSS CONE
MASS
ORBITS
PHOTOMETRY
QUASARS
STARS
TELESCOPES
TWO-BODY PROBLEM