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Related papers: Large-Amplitude X-ray Outbursts from Galactic Nucl…

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Luminous X-ray outbursts with variability amplitudes as high as ~1000 have been detected from a small number of galactic nuclei. These events are likely associated with transient fueling of nuclear supermassive black holes. In this paper,…

Astrophysics · Physics 2009-11-13 B. Luo , W. N. Brandt , A. T. Steffen , F. E. Bauer

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

The luminosity function of active galactic nuclei has been measured down to luminosities ~10^{42} erg/s in the soft and hard X-rays. Some fraction of this activity is associated with the accretion of the material liberated by the tidal…

Astrophysics · Physics 2008-11-26 Milos Milosavljevic , David Merritt , Luis C. Ho

It has long been suggested that supermassive black holes in non-active galaxies might be tracked down by occasional tidal disruptions of stars on nearly radial orbits. A tidal disruption event would reveal itself by a luminous flare of…

Astrophysics · Physics 2009-11-07 Stefanie Komossa

We performed a systematic search for stellar tidal disruption events (TDE) by looking for X-ray sources that were detected during the ROSAT All Sky Survey and faded by more than an order of magnitude over the next two decades according to…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Ildar Khabibullin , Sergey Sazonov

In recent years, giant amplitude X-ray flares have been observed from a handful of non-active galaxies. The most plausible scenario of these unusual phenomena is tidal disruption of a star by a quiescent supermassive black hole at the…

Tidal disruption events of stars by supermassive black holes have so far been discovered months to years after the fact. In this paper we explore the short, faint and hard burst of radiation is emitted at maximum compression, as a result of…

High Energy Astrophysical Phenomena · Physics 2018-10-24 Almog Yalinewich , James Guillochon , Re'em Sari , Abraham Loeb

(abridged) Huge amplitude X-ray outbursts in a few galaxies were reported in the last few years. As one of the exciting possibilities to explain these observations, tidal disruption of a star by a supermassive black hole has been proposed.…

Astrophysics · Physics 2007-05-23 Stefanie Komossa , Norbert Bade

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

Tidal disruption of stars by massive black holes produce transient accretion flows that flare at optical, UV, and X-ray wavelengths. At late times, these accretion flows may launch relativistic jets that can be detected through the…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Geoffrey C. Bower

Large-amplitude, high-luminosity soft X-ray flares were detected by the ROSAT All-Sky Survey in several galaxies with no evidence of Seyfert activity in their ground-based optical spectra. These flares had the properties predicted for a…

Astrophysics · Physics 2016-08-30 J. P. Halpern , S. Gezari , S. Komossa

We compute rates of tidal disruption of stars by supermassive black holes in galactic nuclei, using downwardly-revised black hole masses from the M-sigma relation. In galaxies with steep nuclear density profiles, which dominate the overall…

Astrophysics · Physics 2009-11-07 Jianxiang Wang , David Merritt

Owing to their thermal emission, tidal disruption events (TDEs) were regularly detected in the soft X-rays and sometimes in the optical. Only a few TDEs have been detected at hard X-rays: two are high redshift beamed events, one of which…

High Energy Astrophysical Phenomena · Physics 2016-01-20 Krzysztof Hryniewicz , Roland Walter

During a close encounter between a star and a supermassive black hole, the star can get disrupted by the black hole's tidal forces, resulting in a tidal disruption event (TDE). The accretion of the star's material onto the black hole…

High Energy Astrophysical Phenomena · Physics 2022-05-04 J. Hampel , S. Komossa , J. Greiner , T. H. Reiprich , M. Freyberg , T. Erben

We study the properties of galaxies hosting mid-infrared outbursts in the context of a catalog of five hundred thousand galaxies from the Sloan Digital Sky Survey. We find that nuclear obscuration, as inferred by the surrounding dust mass,…

We report an observational estimate of the rate of stellar tidal disruption flares (TDFs) in inactive galaxies, based on a successful search for these events among transients in galaxies using archival SDSS multi-epoch imaging data (Stripe…

Astrophysics of Galaxies · Physics 2014-08-27 Sjoert van Velzen , Glennys R. Farrar

X-rays are a powerful probe of the physical conditions in the nuclei of active galaxies. We review the X-ray properties of radio-quiet AGN, LINERs and ultraluminous IR galaxies based on observations carried out with the X-ray satellite…

Astrophysics · Physics 2017-08-23 Stefanie Komossa

In the past two decades, high amplitude electromagnetic outbursts have been detected from dormant galaxies and often attributed to the tidal disruption of a star by the central black hole. X-ray emission from the Seyfert 2 galaxy GSN 069…

Tidal forces close to massive black holes can violently disrupt stars that make a close approach. These extreme events are discovered via bright X-ray and optical/UV flares in galactic centers. Prior studies based on modeling decaying flux…

It has been suggested that an unavoidable consequence of the existence of supermassive black holes, and the best diagnostic of their presence in non-active galaxies, would be occasional tidal disruption of stars captured by the black holes.…

Astrophysics · Physics 2009-11-10 S. Komossa , J. Halpern , N. Schartel , G. Hasinger , M. Santos-Lleo , P. Predehl
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