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相关论文: A Tidal Flare Candidate in Abell 1795

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Diffuse radio emission in galaxy clusters, and their connection with cluster mergers, are still debated. We seek to explore the internal dynamics of the radio halo cluster Abell 545. This cluster is also peculiar for hosting in its center a…

宇宙学与河外天体物理 · 物理学 2018-01-17 R. Barrena , M. Girardi , W. Boschin , S. De Grandi , D. Eckert , M. Rossetti

Off-axis collisions between galaxy clusters may induce the phenomenon of sloshing, causing dense gas to be dragged from the cool core of a cluster, resulting in a spiral of enhanced X-ray emission. Abell 2199 displays signatures of sloshing…

Tidal Disruption Events (TDEs) have long been hypothesized as valuable indicators of black holes, offering insight into their demographics and behaviour out to high redshift. TDEs have also enabled the discovery of a few Massive Black Holes…

X-ray Quasi-Periodic Eruptions (QPEs) are a recently discovered phenomenon associated with supermassive black holes at the centers of galaxies. They are high amplitude soft X-ray flares that recur on timescales of hours, but what causes…

高能天体物理现象 · 物理学 2021-11-17 Joheen Chakraborty , Erin Kara , Megan Masterson , Margherita Giustini , Giovanni Miniutti , Richard Saxton

We report a multiwavelength (X-ray, ultraviolet/optical/infrared, radio) analysis of the relativistic tidal disruption event candidate Sw J2058+05 from 3 months to 3 yr post-discovery in order to study its properties and compare its…

We report on a 120 ks XMM-Newton observation of the galaxy cluster Abell 2597. Results from both the European Photon Imaging Camera (EPIC) and the Reflection Grating Spectrometer (RGS) are presented. From EPIC we obtain radial profiles of…

天体物理学 · 物理学 2009-09-17 R. Glenn Morris , A. C. Fabian

NGC 247 is a nearby late-type bulgeless spiral galaxy that contains an inactive nucleus. We report a serendipitous discovery of an X-ray flare from the galaxy center with a luminosity up to 2*10^39 erg/s in the 0.3-10 keV band with…

高能天体物理现象 · 物理学 2015-07-15 Hua Feng , Luis C. Ho , Philip Kaaret , Lian Tao , Kazutaka Yamaoka , Shuo Zhang , Fabien Grisé

We present an analysis of the Chandra X-ray observation of Abell 2052, including large scale properties of the cluster as well as the central region which includes the bright radio source, 3C 317. We present temperature and abundance…

天体物理学 · 物理学 2011-07-18 Elizabeth L. Blanton , Craig L. Sarazin , Brian R. McNamara

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…

高能天体物理现象 · 物理学 2016-01-20 Krzysztof Hryniewicz , Roland Walter

X-ray transients appeared in optically non-active galactic nuclei have been observed in recent years. The most popular model explaining this kind of phenomena is the conventional tidal disruption model. In this model, when a star moves…

天体物理学 · 物理学 2009-06-23 A. Y. L. Wong , Y. F. Huang , K. S. Cheng

An extremely soft X-ray excess throughout galaxy clusters has been claimed as a new feature of these sytems, with important physical implications. We have reexamined this feature in the five clusters for which it has been discussed, using…

天体物理学 · 物理学 2009-10-31 John S. Arabadjis , Joel N. Bregman

The cluster Abell 2199 is one of the prototypical ``cooling flow'' clusters. Its central cD galaxy is host to a steep-spectrum radio source, of the type associated with cooling cores. In this paper we combine radio data with new ROSAT HRI…

天体物理学 · 物理学 2009-10-30 F. N. Owen , J. A. Eilek

We report on X-ray observations made with the Rossi X-ray Timing Explorer of the black hole candidate (BHC) transient XTE J1650-500 at the end of its first, and currently only, outburst. By monitoring the source at low luminosities over…

天体物理学 · 物理学 2008-11-26 John A. Tomsick , Emrah Kalemci , Stephane Corbel , Philip Kaaret

Identification of Abell 3120 as a galaxy cluster has recently been questioned with alternative suggestions including: a fossil remnant of a group merger, non-thermal emission from a radio galaxy, and projected emission from of a filamentary…

宇宙学与河外天体物理 · 物理学 2011-02-11 Mark Henriksen , Alexis Finoguenov

AT 2018hyz (=ASASSN-18zj) is a tidal disruption event (TDE) located in the nucleus of a quiescent E+A galaxy at a redshift of $z = 0.04573$, first detected by the All-Sky Automated Survey for Supernovae (ASAS-SN). We present optical+UV…

We report on observations of black hole Swift J1357.2-0933, a member of the modest population of very faint X-ray transients. This source has previously shown intense dips in the optical lightcurve, a phenomena that has been linked to the…

We present a new analysis of very deep Chandra observations of the galaxy cluster Abell 1795. Utilizing nearly 750 ks of net ACIS imaging, we are able to resolve the thermodynamic structure of the Intracluster Medium (ICM) on length scales…

星系天体物理 · 物理学 2015-06-22 S. Ehlert , M. McDonald , E. D. Miller , L. P. David , M. W. Bautz

Tidal disruption events (TDEs) occur when a star passes close enough to a galaxy's supermassive black hole to be disrupted by tidal forces. We discuss new observations of IGRJ12580+0134, a TDE observed in NGC 4845 (d=17 Mpc) in November…

CSS100217 is considered a peculiar tidal disruption event (TDE) candidate occurring in an active galactic nucleus (AGN). Unlike typical TDEs, where the post-flare luminosity is equal to that pre-flare, CSS100217 decayed to $\sim$ 0.4…

高能天体物理现象 · 物理学 2025-10-01 Ying Gu , Xiao Li , Xing-Qian Cheng , Dou-Dou Wang , Xue-Guang Zhang , En-Wei Liang

We have searched for diffuse intracluster light in the galaxy cluster Abell 2667 (z=0.233) from HST images in three filters. We have applied to these images an iterative multi-scale wavelet analysis and reconstruction technique, which…

天体物理学 · 物理学 2009-11-11 G. Covone , C. Adami , F. Durret , J. -P. Kneib , G. B. Lima Neto , E. Slezak