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Related papers: Multiwavelength Study of an X-ray Tidal Disruption…

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We study X-ray bright tidal disruption events (TDE), close to the peak of their emission, with the intention of understanding the evolution of their light curves and spectra. Candidate TDE are identified by searching for soft X-ray flares…

Astrophysics of Galaxies · Physics 2017-02-01 R. D. Saxton , A. M. Read , S. Komossa , P. Lira , K. D. Alexander , M. H. Wieringa

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…

The ultrasoft X-ray flare 2XMMi J184725.1-631724 was serendipitously detected in two XMM-Newton observations in 2006 and 2007, with a peak luminosity of 6X10^43 erg/s. It was suggested to be a tidal disruption event (TDE) because its…

High Energy Astrophysical Phenomena · Physics 2017-12-27 Dacheng Lin , Jay Strader , Eleazar R. Carrasco , Olivier Godet , Dirk Grupe , Natalie A. Webb , Didier Barret , Jimmy A. Irwin

We present the discovery of a luminous X-ray transient, serendipitously detected by Swift's X-ray Telescope (XRT) on 2020 February 5, located in the nucleus of the galaxy SDSS J143359.16+400636.0 at z=0.099 (luminosity distance $D_{\rm…

We have discovered an ultrasoft X-ray transient source, 2XMMi J184725.1-631724, which was detected serendipitously in two XMM-Newton observations in the direction of the center of the galaxy IC 4765-f01-1504 at a redshift of 0.0353. These…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Dacheng Lin , Eleazar R. Carrasco , Dirk Grupe , Natalie A. Webb , Didier Barret , Sean A. Farrell

We report on the discovery of an ultrasoft X-ray transient source, 3XMM J152130.7+074916. It was serendipitously detected in an XMM-Newton observation on 2000 August 23, and its location is consistent with the center of the galaxy SDSS…

High Energy Astrophysical Phenomena · Physics 2015-09-23 Dacheng Lin , Peter W. Maksym , Jimmy A. Irwin , S. Komossa , Natalie A. Webb , Olivier Godet , Didier Barret , Dirk Grupe , Stephen D. J. Gwyn

Aims. We investigate the evolution of X-ray selected tidal disruption events. Methods. New events are found in near-real time data from XMM-Newton slews and are monitored by multi-wavelength facilities. Results. In August 2016, X-ray…

High Energy Astrophysical Phenomena · Physics 2019-10-02 R. D. Saxton , A. M. Read , S. Komossa , P. Lira , K. D. Alexander , I. Steele , F. Ocaña , E. Berger , P. Blanchard

As part of our ongoing archival X-ray survey of galaxy clusters for tidal flares, we present evidence of an X-ray transient source within 1 arcmin of the core of Abell 1795. The extreme variability (a factor of nearly 50), luminosity (> 2 x…

High Energy Astrophysical Phenomena · Physics 2013-09-23 W. P. Maksym , M. P. Ulmer , M. C. Eracleous , L. Guennou , L. C. Ho

The X-ray source 3XMM~J150052.0+015452 was discovered as a spectacular tidal disruption event candidate during a prolonged ($>11$ yrs) outburst (Lin et al. 2017). It exhibited unique quasi-soft X-ray spectra of characteristic temperature…

New high variability extragalactic sources may be identified by comparing the flux of sources seen in the XMM-Newton Slew Survey with detections and upper limits from the ROSAT All Sky Survey. In November 2012, X-ray emission was detected…

High Energy Astrophysical Phenomena · Physics 2014-11-19 R. D. Saxton , A. M. Read , S. Komossa , P. Rodriguez-Pascual , G. Miniutti , P. Dobbie , P. Esquej , M. Colless , K. W. Bannister

The X-ray source 2XMM J123103.2+110648 was previously found to show pure thermal X-ray spectra and a ~3.8 hr periodicity in three XMM-Newton X-ray observations in 2003-2005, and the optical spectrum of the host galaxy suggested it as a type…

High Energy Astrophysical Phenomena · Physics 2017-04-12 Dacheng Lin , Olivier Godet , Luis C. Ho , Didier Barret , Natalie A. Webb , Jimmy A. Irwin

We present the results of the first broadband X-ray analysis of the ultraluminous X-ray source NGC 5055 ULX X-1, combining simultaneous data from XMM$-$Newton and NuSTAR missions, with a combined exposure time of $\sim$100 ks across the…

High Energy Astrophysical Phenomena · Physics 2025-11-18 N. Cruz-Sanchez , E. A. Saavedra , F. A. Fogantini , F. García , J. A. Combi

We report here on observations of a tidal disruption event, XMMSL2 J1404-2511, discovered in an XMM-Newton slew, in a quiescent galaxy at z=0.043. X-ray monitoring covered the epoch when the accretion disc transitioned from a thermal state,…

High Energy Astrophysical Phenomena · Physics 2026-01-14 R. D. Saxton , T. Wevers , S. van Velzen , K. Alexander , Z. Liu , A. Mummery , M. Giustini , G. Miniutti , F. Fuerst , J. J. E. Kajava , A. M. Read , P. G. Jonker , A. Rau , D. -Y. Li

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

XMM-Newton EPIC observations have revealed a bright point-like X-ray source in the nearby Magellanic-type galaxy NGC 55. At the distance of NGC 55, the maximum observed X-ray luminosity of the source, designated as XMMU J001528.9-391319, is…

Astrophysics · Physics 2009-11-10 A-M. Stobbart , T. P. Roberts , R. S. Warwick

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

Tidal disruption events (TDEs), which occur when stars enter the tidal radii of supermassive black holes (SMBHs) and are subsequently torn apart by their tidal forces, represent intriguing phenomena that stimulate growing research interest…

While the vast majority of Tidal Disruption Events (TDEs) has been identified by wide-field sky surveys in the optical and X-ray bands, recent studies indicate that a considerable fraction of TDEs may be dust obscured, and thus…

We present the most extensive high-time resolution multi-band campaign to date on the candidate transitional millisecond pulsar (tMSP) 3FGL J1544.6-1125 in the sub-luminous disk state, with coordinated observations from the radio to the…

We report the X-ray data analysis of two transient ultraluminous X-ray sources (ULXs, hereafter X1 and X2) located in the nearby galaxy NGC 7090. While they were not detected in the 2004 XMM-Newton and 2005 Chandra observations, their…

High Energy Astrophysical Phenomena · Physics 2019-05-08 Zhu Liu , P. T. O'Brien , J. P. Osborne , P. A. Evans , K. L. Page
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