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相关论文: Ultra-luminous X-ray Sources in nearby galaxies fr…

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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

Ultraluminous X-ray sources (ULXs) are mostly extragalactic non-nuclear point sources having X-ray luminosity exceeding the Eddington luminosity of 10 $M_\odot$ black hole i.e., $L_X \geq $ 10$^{39}$ erg ~s$^{-1}$. They are observed in all…

高能天体物理现象 · 物理学 2026-05-08 C. M. Sariga , P. Shalima , D. Bhattacharya , Vivek K. Agrawal

Ultraluminous X-ray sources (ULXs) are amongst the most intriguing of X-ray source classes. Their extreme luminosities - greater than 10^39 erg/s in the 0.3 - 10 keV band alone - suggest either the presence of black holes larger than those…

天体物理学 · 物理学 2008-11-26 T. P. Roberts

We present some results from an archival VLA study of ultraluminous X-ray source s (ULXs). These unresolved non-nuclear X-ray sources have luminosities (L_X >= 1 0^39 ergs/sec) which may require somewhat exotic explanations, such as…

天体物理学 · 物理学 2007-05-23 Neal A. Miller , Susan G. Neff , Richard F. Mushotzky

Since their discovery, Ultraluminous X-ray sources (ULXs) have attracted attention due to their combination of extreme luminosities and extra-nuclear locations. However, they are a fairly rare phenomenon, and attempts to investigate the…

高能天体物理现象 · 物理学 2015-05-20 D. J. Walton , J. C. Gladstone , T. P. Roberts , A. C. Fabian

One hundred fifty-four discrete non-nuclear Ultra-Luminous X-ray (ULX) sources, with intrinsic X-ray luminosities >1e39 ergs/s, are identified in 82 galaxies observed with Chandra's Advanced CCD Imaging Spectrometer. Source positions, X-ray…

天体物理学 · 物理学 2009-11-10 Douglas A. Swartz , Kajal K. Ghosh , Allyn F. Tennant , Kinwah Wu

We present the results from an X-ray and optical study of a new sample of eight extreme luminosity ultraluminous X-ray source (ULX) candidates, which were selected as the brightest ULXs (with L_X > 5x10^40 erg/s) located within 100 Mpc…

高能天体物理现象 · 物理学 2015-06-04 Andrew D. Sutton , Timothy P. Roberts , Dominic J. Walton , Jeanette C. Gladstone , Amy E. Scott

Ultraluminous X-ray sources (ULX) are off-nuclear point sources in nearby galaxies whose X-ray luminosity exceeds the theoretical maximum for spherical infall (the Eddington limit) onto stellar-mass black holes. Their luminosity ranges from…

The nature of ultra-luminous X-ray sources (ULXs), which are off-nuclear extragalactic X-ray sources that exceed the Eddington luminosity for a stellar-mass black hole, is still largely unknown. They might be black hole X-ray binaries in a…

高能天体物理现象 · 物理学 2013-02-20 Mathieu Servillat , Alexis Coleiro , Sylvain Chaty

One hundred seven ultraluminous X-ray (ULX) sources with 0.3-10.0 keV luminosities in excess of 1e39 erg/s are identified in a complete sample of 127 nearby galaxies. The sample includes all galaxies within 14.5 Mpc above the completeness…

高能天体物理现象 · 物理学 2015-05-30 Douglas A. Swartz , Roberto Soria , Allyn F. Tennant , Mihoko Yukita

The extreme extragalactic sources known as Ultraluminous X-ray Sources (ULX) represent a unique testing environment for compact objects population studies and the accretion process. Their nature has long been disputed. Their luminosity,…

高能天体物理现象 · 物理学 2016-04-18 Matteo Bachetti

The premise that Ultraluminous X-ray sources (ULXs) exist beyond the optical extent of nearby galaxies is investigated. A published catalog containing 41 ULX candidates located between 1 and ~3 times the standard D_{25} isophotal radius of…

天体物理学 · 物理学 2011-02-11 Douglas A. Swartz

Ultraluminous X-ray sources (ULXs) represent a class of binary systems that are more luminous than any black hole in our Galaxy. The nature of these objects remained unclear for a long time. The most popular models for the ULXs involve…

高能天体物理现象 · 物理学 2018-12-07 Kirill Atapin

We present results of a Chandra survey of the ultra-luminous X-ray sources (ULX) in 13 normal galaxies, in which we combine source detection with X-ray flux measurement. 22 ULX were detected, i.e. with L_x > 1 x 10^{39} erg s^{-1} (L_10),…

天体物理学 · 物理学 2009-09-29 P. J. Humphrey , G. Fabbiano , M. Elvis , M. J. Church , M. Balucinska-Church

Ultraluminous X-ray sources (ULXs) are a population of extragalactic objects whose luminosity exceeds the Eddington limit for a 10 Msun black hole (BH). Their properties have been widely interpreted in terms of accreting stellar-mass or…

高能天体物理现象 · 物理学 2017-02-22 F. Pintore , L. Zampieri , L. Stella , A. Wolter , S. Mereghetti , G. L. Israel

We have created a new, clean catalogue of extragalactic non-nuclear X-ray sources by correlating the 3XMM-DR4 data release of the XMM-Newton Serendipitous Source Catalogue with the Third Reference Catalogue of Bright Galaxies and the…

高能天体物理现象 · 物理学 2019-01-09 H. P. Earnshaw , T. P. Roberts , M. J. Middleton , D. J. Walton , S. Mateos

The statistical properties of the ultra-luminous X-ray source (ULX) populations extracted from the ROSAT HRI survey of X-ray point sources in nearby galaxies in Paper I are studied to reveal connections between the ULX phenomenon and survey…

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

Ultra-/hyper-luminous X-ray sources (ULX/HLX) could be interesting laboratories to improve our understanding of the supermassive black hole growth through super-Eddington accretion episodes and successive mergers of lighter holes. ULXs are…

高能天体物理现象 · 物理学 2024-01-10 Hugo Tranin , Natalie Webb , Olivier Godet , Erwan Quintin

Ultra-luminous X-ray sources (ULXs) are off-nuclear point sources in nearby galaxies with luminosities well exceeding the Eddington limit for stellar-mass objects. It has been recognized after the discovery of pulsating ULXs (PULXs) that a…

高能天体物理现象 · 物理学 2020-01-22 M. Hakan Erkut , K. Yavuz Ekşi

We have searched for ultraluminous X-ray sources (ULXs) in a sample of 28 elliptical and S0 galaxies observed with Chandra. We find that the number of X-ray sources detected at a flux level that would correspond to a 0.3-10 keV X-ray…

天体物理学 · 物理学 2009-11-10 Jimmy A. Irwin , Joel N. Bregman , Alex E. Athey
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