AT 2021hdr: A candidate tidal disruption of a gas cloud by a binary super massive black hole system
arXiv:2411.08949 · doi:10.1051/0004-6361/202451305
Abstract
With a growing number of facilities able to monitor the entire sky and produce light curves with a cadence of days, in recent years there has been an increased rate of detection of sources whose variability deviates from standard behavior, revealing a variety of exotic nuclear transients. The aim of the present study is to disentangle the nature of the transient AT 2021hdr, whose optical light curve used to be consistent with a classic Seyfert 1 nucleus, which was also confirmed by its optical spectrum and high-energy properties. From late 2021, AT 2021hdr started to present sudden brightening episodes in the form of oscillating peaks in the Zwicky Transient Facility (ZTF) alert stream, and the same shape is observed in X-rays and UV from Swift data. The oscillations occur every about 60-90 days with amplitudes of around 0.2 mag in the g and r bands. Very Long Baseline Array (VLBA) observations show no radio emission at milliarcseconds scale. It is argued that these findings are inconsistent with a standard tidal disruption event (TDE), a binary supermassive black hole (BSMBH), or a changing-look active galactic nucleus (AGN); neither does this object resemble previous observed AGN flares, and disk or jet instabilities are an unlikely scenario. Here, we propose that the behavior of AT 2021hdr might be due to the tidal disruption of a gas cloud by a BSMBH. In this scenario, we estimate that the putative binary has a separation of about 0.83 mpc and would merge in about 70000 years. This galaxy is located at 9 kpc from a companion galaxy, and in this work we report this merger for the first time. The oscillations are not related to the companion galaxy.
arXiv comment11 pages, 5 figures, 2 tables, plus appendices. Accepted for publication in Astronomy & Astrophysics. NASA press release available at https://science.nasa.gov/missions/swift/nasas-swift-studies-gas-churning-monster-black-holes/ doi: 10.1051/0004-6361/202451305
References in corpus (99)
- Gaia Data Release 2. Summary of the contents and survey properties
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- Gaia Data Release 3: Summary of the content and survey properties
- The Swift X-ray Telescope
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- The Swift Ultra-Violet/Optical Telescope
- Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background
- Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
- The Zwicky Transient Facility: Data Processing, Products, and Archive
- On characterising the variability properties of X-ray light curves from active galaxies
- Preliminary Results from NEOWISE: An Enhancement to the Wide-field Infrared Survey Explorer for Solar System Science
- The Zwicky Transient Facility: Science Objectives
- Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe
- Are the Variations in Quasar Optical Flux Driven by Thermal Fluctuations?
- Gaia Early Data Release 3: Photometric content and validation
- Initial Performance of the NEOWISE Reactivation Mission
- The Ensemble Photometric Variability of ~25000 Quasars in the Sloan Digital Sky Survey
- Tidal Disruption Events
- Evolution of massive binary black holes
- The Discovery of the First "Changing Look" Quasar: New Insights into the Physics & Phenomenology of AGN
- A massive binary black-hole system in OJ287 and a test of general relativity
- The 105 month Swift-BAT all-sky hard X-ray survey
- Massive black hole binary mergers within sub-pc scale gas discs
- A possible close supermassive black-hole binary in a quasar with optical periodicity
- Quasar feedback and the origin of radio emission in radio-quiet quasars
- On the X-ray, optical emission line and black hole mass properties of local Seyfert galaxies
- An XMM-Newton spectral survey of 12 micron selected galaxies. I. X-ray data
- A Systematic Search for Changing-Look Quasars in SDSS
- A gas cloud on its way towards the super-massive black hole in the Galactic Centre
- Swift BAT Survey of AGN
- Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus
- Flexible and Scalable Methods for Quantifying Stochastic Variability in the Era of Massive Time-Domain Astronomical Data Sets
- The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
- A Population of Short-Period Variable Quasars from PTF as Supermassive Black Hole Binary Candidates
- The 22-Month Swift-BAT All-Sky Hard X-ray Survey
- Optical-Ultraviolet Tidal Disruption Events
- The Automatic Learning for the Rapid Classification of Events (ALeRCE) Alert Broker
- 1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months
- The Palermo Swift-BAT hard X-ray catalogue III. Results after 54 months of sky survey
- The Radio Spectral Energy Distribution and Star Formation Rate Calibration in Galaxies
- The destruction and recreation of the X-ray corona in a changing-look Active Galactic Nucleus
- Selecting Quasars by their Intrinsic Variability
- The X-ray and Radio Connection in Low-luminosity Active Nuclei
- Tearing up the disc: how black holes accrete
- Bardeen-Petterson Alignment, Jets and Magnetic Truncation in GRMHD Simulations of Tilted Thin Accretion Discs
- Alert Classification for the ALeRCE Broker System: The Light Curve Classifier
- Observing Lense-Thirring Precession in Tidal Disruption Flares
- Understanding extreme quasar optical variability with CRTS: I. Major AGN flares
- ASASSN-14ko is a Periodic Nuclear Transient in ESO 253-G003
- A milliparsec supermassive black hole binary candidate in the galaxy SDSS J120136.02+300305.5
- Quasi-periodic eruptions from impacts between the secondary and a rigidly precessing accretion disc in an extreme mass-ratio inspiral system
- A New Class of Changing-Look LINERs
- Disc Tearing and Bardeen-Petterson Alignment in GRMHD Simulations of Highly Tilted Thin Accretion Discs
- Super-massive binary black holes and emission lines in active galactic nuclei
- A new class of flares from accreting supermassive black holes
- Interacting Stellar EMRIs as Sources of Quasi-Periodic Eruptions in Galactic Nuclei
- Repeating tidal disruptions in GSN 069: Long-term evolution and constraints on quasi-periodic eruptions' models
- Feeding SMBHs through supersonic turbulence and ballistic accretion
- Tidal disruption events in active galactic nuclei
- Massive black hole pairs in clumpy, self-gravitating circumnuclear disks: stochastic orbital decay
- Tidal disruption events from supermassive black hole binaries
- Interruption of Tidal Disruption Flares By Supermassive Black Hole Binaries
- Quasi-Periodic Erupters: A Stellar Mass-Transfer Model for the Radiation
- The Curious Case of ASASSN-20hx: A Slowly-Evolving, UV and X-ray Luminous, Ambiguous Nuclear Transient
- AGN Variability Analysis Handbook
- The complex time and energy evolution of quasi-periodic eruptions in eRO-QPE1
- Unstable Mass Transfer from a Main-Sequence Star to a Supermassive Black Hole and Quasi-Periodic Eruptions
- Sub-parsec radio cores in nearby Seyfert galaxies
- X-ray eruptions every 22 days from the nucleus of a nearby galaxy
- The 450 days X-ray monitoring of the changing-look AGN 1ES 1927+654
- The QUEST-La Silla AGN variability survey: connection between AGN variability and black hole physical properties
- Slow blue nuclear hypervariables in PanSTARRS-1
- Monthly quasi-periodic eruptions from repeated stellar disruption by a massive black hole
- Distinguishing Tidal Disruption Events from Impostors
- ALMA Observations of Massive Clouds in the Central Molecular Zone: Jeans Fragmentation and Cluster Formation
- Fallback Rates from Partial Tidal Disruption Events
- Large-amplitude variables in Gaia Data Release 2. Multi-band variability characterization
- Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results
- Infalling clouds on to supermassive black hole binaries - II. Binary evolution and the final parsec problem
- Long-term Evolution of Binary Orbits Induced by Circumbinary Disks
- Robust period estimation using mutual information for multi-band light curves in the synoptic survey era
- Infalling clouds onto super-massive black hole binaries - I. Formation of discs, accretion and gas dynamics
- The rise and fall of the iron-strong nuclear transient PS16dtm
- A structure function analysis of VST-COSMOS AGN
- Accurate classification of 75 counterparts of objects detected in the 54 month Palermo Swift/BAT hard X-ray catalogue
- Lense-Thirring Precession after a Supermassive Black Hole Disrupts a Star
- Chandra, HST/STIS, NICER, Swift, and TESS Detail the Flare Evolution of the Repeating Nuclear Transient ASASSN-14ko
- Light curves of tidal disruption events in active galactic nuclei
- Tidal disruption of stars in a supermassive black hole binary system: the influence of orbital properties on fallback and accretion rates
- Tidal disruptions in circumbinary discs (I): Star formation, dynamics, and binary evolution
- Optical follow-up of the tick-tock massive black hole binary candidate
- From radio-quiet to radio-silent: low luminosity Seyfert radio cores
- Dissonance in harmony: The UV/optical periodic outbursts of ASASSN-14ko exhibit repeated bumps and rebrightenings
- The Swansong of the Galactic Center Source X7: An Extreme Example of Tidal Evolution near the Supermassive Black Hole
- TDE fallback cut-off due to a pre-existing accretion disc
- A Multiband Generalization of the Analysis of Variance Period Estimation Algorithm and the Effect of Inter-band Observing Cadence on Period Recovery Rate
- Multiwavelength monitoring of the nucleus in PBC J2333.9-2343: the giant radio galaxy with a blazar-like core
- Multiwavelength analysis and the C IV λ1549 Å emission line behavior from 2008 to 2020 of the FSRQ B2 1633+382
- Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars