The first systematically identified repeating partial tidal disruption event
Jean J. Somalwar, Vikram Ravi, Yuhan Yao, Muryel Guolo, Matthew, Graham, Erica Hammerstein, Wenbin Lu, Matt Nicholl, Yashvi Sharma, Robert, Stein, Sjoert van Velzen, Eric C. Bellm, Michael W. Coughlin, Steven L., Groom, Frank J. Masci, Reed Riddle

TL;DR
This paper reports the first systematic identification of a repeating partial tidal disruption event, AT 2020vdq, providing new insights into TDE mechanisms and rates in galactic nuclei.
Contribution
It presents the discovery and analysis of the first systematically identified repeating pTDE, constraining models and the binary fraction in galactic centers.
Findings
AT 2020vdq is confirmed as a repeating pTDE.
The repeating pTDE rate is estimated at 10^{-6} to 10^{-5} per galaxy per year.
The data suggest a few percent binary fraction in galactic nuclei.
Abstract
Tidal disruption events (TDEs) occur when a star enters the tidal radius of a supermassive black hole (SMBH). If the star only grazes the tidal radius, a fraction of the stellar mass will be accreted in a partial TDE (pTDE). The remainder can continue orbiting and may re-disrupted at pericenter, causing a repeating pTDE. pTDEs may be as or more common than full TDEs (fTDEs), yet few are known. In this work, we present the discovery of the first repeating pTDE from a systematically-selected sample, AT\,2020vdq. AT\,2020vdq was originally identified as an optically- and radio-flaring TDE. Around years after its discovery, it rebrightened dramatically and rapidly in the optical. The optical flare was remarkably fast and luminous compared to previous TDEs. It was accompanied by extremely broad () optical/UV spectral features and faint X-ray emission ($L_X \sim…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Mechanics and Biomechanics Studies · Sports Dynamics and Biomechanics
