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Related papers: Unbeamed tidal disruption events at hard X-rays

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X-ray and $\gamma$-ray observations by the Swift satellite revealed that a fraction of tidal disruption events (TDEs) have relativistic jets. Jetted TDEs have been considered as potential sources of very high-energy cosmic-rays and…

High Energy Astrophysical Phenomena · Physics 2017-04-03 Nicholas Senno , Kohta Murase , Peter Meszaros

Observational consequences of tidal disruption of stars (TDEs) by supermassive black holes (SMBHs) can enable us to discover quiescent SMBHs, constrain their mass function, study formation and evolution of transient accretion disks and jet…

High Energy Astrophysical Phenomena · Physics 2015-06-23 I. Donnarumma , E. M. Rossi

In this work, we use the Jansky VLA Sky Survey (VLASS) to compile the first sample of six radio-selected tidal disruption events (TDEs) with transient optical counterparts. While we still lack the statistics to do detailed population…

The discovery of optical/UV tidal disruption events (TDEs) was surprising. The expectation was that, upon returning to the pericenter, the stellar-debris stream will form a compact disk that will emit soft X-rays. Indeed the first TDEs were…

High Energy Astrophysical Phenomena · Physics 2021-02-03 Tatsuya Matsumoto , Tsvi Piran

A unique signature for the presence of massive black holes in very dense stellar regions is occasional giant-amplitude outbursts of multiwavelength radiation from tidal disruption and subsequent accretion of stars that make a close approach…

Tidal disruption events (TDEs) have traditionally been discovered in optical sky surveys through targeted searches of nuclear transients. However, it is expected that some TDEs will occur outside the galaxy nucleus, arising from wandering…

We present late-time observations by Swift and XMM-Newton of the tidal disruption event (TDE) ASASSN-15oi that reveal that the source brightened in the X-rays by a factor of $\sim10$ one year after its discovery, while it faded in the…

High Energy Astrophysical Phenomena · Physics 2017-12-27 S. Gezari , S. B. Cenko , I. Arcavi

Tidal disruption events which repeat on timescales of months-to-years represent an unambiguous signature of a partial disruption, with the surviving stellar remnant returning to pericentre to be repeatedly stripped by tidal forces. These…

High Energy Astrophysical Phenomena · Physics 2026-02-24 Andrew Mummery

One efficient method to probe the direct vicinity of SMBHs in nearby galaxies is to make use of the detection of flares from tidally disrupted stars (e.g., Lidskii & Ozernoi 1979, Rees 1988). The first few excellent candidates for the…

Astrophysics · Physics 2007-05-23 Stefanie Komossa

About a hundred tidal disruption events (TDEs) have been observed and they exhibit a wide range of emission properties both at peak and over their lifetimes. Some TDEs peak predominantly at X-ray energies while others radiate chiefly at UV…

High Energy Astrophysical Phenomena · Physics 2022-10-05 Lars Lund Thomsen , Tom Kwan , Lixin Dai , Samantha Wu , Enrico Ramirez-Ruiz

Tidal disruption events (TDEs) are bursts of electromagnetic energy released when supermassive black holes (SMBHs) at the centers of galaxies violently disrupt a star that passes too close. TDEs provide a new window to study accretion onto…

We perform the first systematic study of the minute-to-hours-timescale stochastic variability observed in the X-ray luminosity of tidal disruption events (TDEs) using XMM-Newton data and Fourier analysis methods. We measure the spectral…

High Energy Astrophysical Phenomena · Physics 2026-02-20 Joheen Chakraborty , Megan Masterson , Andrew Mummery , Erin Kara , Christos Panagiotou , Riccardo Arcodia , Vera Berger

The process of tidal disruption of stars by a supermassive black hole (SMBH) provides luminous UV and soft X-ray flares with peak luminosities of $\approx 10^{46}$ ergs/sec and duration of a few months. As part of a wider exploration of the…

High Energy Astrophysical Phenomena · Physics 2019-04-17 Andrea Sacchi , Giuseppe Lodato

In this Letter, we report the detection of soft X-ray time lags-i.e. variability in the softer photons lagging behind that in the harder photons-in seven XMM-Newton observations of the tidal disruption event (TDE) candidate AT2021ehb. We…

High Energy Astrophysical Phenomena · Physics 2026-01-21 Wenjie Zhang

We present a systematic analysis of the radio properties of an X-ray selected sample of tidal disruption event (TDE) candidates discovered by the eROSITA telescope. We find radio sources coincident with half of the transient events (11…

High Energy Astrophysical Phenomena · Physics 2025-04-15 A. J. Goodwin , M. Burn , G. E. Anderson , J. C. A. Miller-Jones , I. Grotova , P. Baldini , Z. Liu , A. Malyali , A. Rau , M. Salvato

In the last few years, giant-amplitude, non-recurrent X-ray flares have been observed from several non-active galaxies (NGC 5905, RXJ1242-11, RXJ1624+75, RXJ1420+53, RXJ1331-32). All of them share similar properties, namely: extreme X-ray…

Astrophysics · Physics 2016-08-30 Stefanie Komossa , Michael Dahlem

AT2022cmc was recently reported as the first on-axis jetted tidal disruption event (TDE) discovered in the last decade, and the fourth on-axis jetted TDE candidate known so far. In this work, we present NuSTAR hard X-ray (3--30 keV)…

High Energy Astrophysical Phenomena · Physics 2024-02-22 Yuhan Yao , Wenbin Lu , Fiona Harrison , S. R. Kulkarni , Suvi Gezari , Muryel Guolo , S. Bradley Cenko , Anna Y. Q. Ho

The concept of stars being tidally ripped apart and consumed by a massive black hole (MBH) lurking in the center of a galaxy first captivated theorists in the late 1970's. The observational evidence for these rare but illuminating phenomena…

High Energy Astrophysical Phenomena · Physics 2021-11-15 Suvi Gezari

Rates of stellar tidal disruption events (TDEs) by supermassive black holes (SMBHs) due to two-body relaxation are calculated using a large galaxy sample (N=146) in order to explore the sensitivity of the TDE rates to observational…

High Energy Astrophysical Phenomena · Physics 2016-02-26 Nicholas C. Stone , Brian D. Metzger