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相关论文: Optical study of the hyper-luminous X-ray source 2…

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Ultra-luminous X-Ray sources are extra-nuclear point sources in external galaxies with $L_X=10^{39}$--$10^{41}$ erg/s and are among the most poorly understood X-ray sources. To help understand their nature, we are trying to identify their…

天体物理学 · 物理学 2009-11-10 Ji-Feng Liu Joel N. Bregman , Patrick Seitzer

We report on the identification of the optical and infrared counterparts of the ultraluminous X-ray source (ULX) XMMU J121214.5+131248 (NGC4168-ULX1). The optical spectrum yields a redshift of z=0.217, which implies that the ULX is not…

天体物理学 · 物理学 2009-11-07 N. Masetti , L. Foschini , L. C. Ho , M. Dadina , G. Di Cocco , G. Malaguti , E. Palazzi

We report the identification of the optical counterpart to the transient ultraluminuos X-ray source in the blue dwarf galaxy UGC6456 (VII Zw 403). The source is highly variable in both the X-ray (more 100 times, 0.3-10 keV) and optical…

高能天体物理现象 · 物理学 2020-10-13 Alexander Vinokurov , Kirill Atapin , Yulia Solovyeva

We studied the multiband properties of two ultraluminous X-ray sources (2CXO J225728.9-410211 = X-1 and 2CXO J225724.7-410343 = X-2) and their surroundings, in the spiral galaxy NGC 7424. Both sources have approached X-ray luminosities…

高能天体物理现象 · 物理学 2024-02-16 Roberto Soria , Siying Cheng , Manfred W. Pakull , Christian Motch , Thomas D. Russell

We report the discovery of a new ultraluminous X-ray source (ULX) in the nearby galaxy NGC 4244 from Chandra archival data. The source, 1WGAJ1216.9+3743, is one of the least luminous and softest ULXs discovered so far. Its X-ray spectrum is…

天体物理学 · 物理学 2009-11-07 I. Cagnoni , R. Turolla , A. Treves , J. -S. Huang , D. W. Kim , M. Elvis , A. Celotti

We report on six Chandra and one HST/WFC3 observation of CXO J122518.6+144545, discovered by Jonker et al. (2010) as a candidate hyperluminous X-ray source (HLX), X-ray bright supernova or recoiling supermassive black hole at $L_X = 2.2…

高能天体物理现象 · 物理学 2015-09-30 M. Heida , P. G. Jonker , M. A. P. Torres

We present Very Large Telescope/X-shooter and Chandra X-ray observatory/ACIS observations of the ULX [SST2011] J110545.62+000016.2 in the galaxy NGC 3521. The source identified as a candidate near-infrared counterpart to the ULX in our…

高能天体物理现象 · 物理学 2019-08-14 K. M. López , P. G. Jonker , M. Heida , M. A. P. Torres , T. P. Roberts , D. J. Walton , D. -S. Moon , F. A. Harrison

We report the discovery of a new ultraluminous X-ray source (ULX) 2XMM J125048.6+410743 within the spiral galaxy M94. The source has been observed by ROSAT, Chandra, and XMM-Newton on several occasions, exhibiting as a highly variable…

高能天体物理现象 · 物理学 2015-06-17 Dacheng Lin , Jimmy A. Irwin , Natalie A. Webb , Didier Barret , Ronald A. Remillard

Despite much observational and theoretical effort little is presently known about the nature of the luminous non-nuclear X-ray sources which appear to largely surpass the Eddington limit of a few solar masses. Here we present first results…

天体物理学 · 物理学 2007-05-23 Manfred W. Pakull , Laurent Mirioni

We study the X-ray and optical properties of the ultraluminous X-ray source (ULX) X-6 in the nearby galaxy NGC 4258 (M106) based on the archival {\it XMM-Newton}, {\it Chandra}, {\it Swift}, and {\it Hubble Space Telescope} ({\it HST})…

高能天体物理现象 · 物理学 2016-09-22 Hasan Avdan , Senay Avdan , Aysun Akyuz , Solen Balman , Nazim Aksaker , Inci Akkaya Oralhan

We report results from Hubble Space Telescope WFPC2 imaging of the field of the luminous, bursting X-ray source in the globular cluster NGC 6441. Although the X-ray position is known to a precision of a few arcseconds, this source is only…

天体物理学 · 物理学 2009-10-30 Eric W. Deutsch , Scott F. Anderson , Bruce Margon , Ronald A. Downes

In this Paper we report the discovery of CXO J122518.6+144545; a peculiar X-ray source with a position 3.6+-0.2",off-nuclear from an SDSS DR7 z=0.0447 galaxy. The 3.6" offset corresponds to 3.2 kpc at the distance of the galaxy. The 0.3-8…

高能天体物理现象 · 物理学 2015-05-18 P. G. Jonker , M. A. P. Torres , A. C. Fabian , M. Heida , G. Miniutti , D. Pooley

We report on Chandra observations of the bright ultra-luminous X-ray (ULX) source in NGC3921. Previous XMM observations reported in the literature show the presence of a bright ULX at a 0.5-10 keV luminosity of 2x10^40 erg/s. Our Chandra…

We report the serendipitous discovery of several unresolved X-ray sources lying in the prominent spiral arms of the galaxy KUG 0214-057 in XMM-Newton observations. The location of these X-ray sources strongly suggests that at least three,…

天体物理学 · 物理学 2009-11-11 M. G. Watson , T. P. Roberts , M. Akiyama , Y. Ueda

The existence of black holes of masses ~ 10^2-10^5 Msun has important implications for the formation and evolution of star clusters and supermassive black holes. One of the strongest candidates to date is the hyperluminous X-ray source…

高能天体物理现象 · 物理学 2015-05-14 Roberto Soria , George K. T. Hau , Alister W. Graham , Albert K. H. Kong , N. Paul M. Kuin , I-Hui Li , Ji-Feng Liu , Kinwah Wu

We present radio through X-ray results of a bright (10^{40} erg/s in the 0.5 to 8.0 keV band) ultraluminous X-ray source (ULX), CXOU J153434.9+151149, in the starburst, interacting pair of galaxies NGC 5953/5954. Chandra image of this ULX…

天体物理学 · 物理学 2009-11-13 Margarita Rosado , Kajal K. Ghosh , Isaura Fuentes-Carrera

Ultraluminous X-ray sources (ULXs) are some of the most enigmatic X-ray bright sources known to date. It is generally accepted that they cannot host black holes as large as those associated with active galaxies, but they appear to be…

高能天体物理现象 · 物理学 2015-05-28 D. J. Walton , T. P. Roberts , S. Mateos , V. Heard

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…

高能天体物理现象 · 物理学 2019-05-08 Zhu Liu , P. T. O'Brien , J. P. Osborne , P. A. Evans , K. L. Page

Archival {\it XMM-Newton}, {\it Chandra} and {\it Hubble Space Telescope (HST)} data have been used to study the X-ray and optical properties of two candidate ultraluminous X-ray sources (ULXs) in NGC\,4536. In order to search for potential…

We report the identification of the optical and radio counterparts of the ultraluminous X-ray (ULX) source XMMU J124825.9+083020 (NGC4698-ULX1). The optical spectrum taken with the VLT yields a redshift of z=0.43, which implies that the ULX…

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