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Ultraluminous x-ray sources (ULXs) in nearby galaxies shine brighter than any X-ray source in our Galaxy. ULXs are usually modeled as stellar-mass black holes (BHs) accreting at very high rates or intermediate-mass BHs. We present…

X-ray observations have revealed in other galaxies a class of extra-nuclear X-ray point sources with X-ray luminosities of $10^{39}$--$10^{41}$ erg/sec, exceeding the Eddington luminosity for stellar mass X-ray binaries. These…

Astrophysics · Physics 2009-11-10 Ji-Feng Liu , Joel N. Bregman

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…

Astrophysics · Physics 2009-11-07 I. Cagnoni , R. Turolla , A. Treves , J. -S. Huang , D. W. Kim , M. Elvis , A. Celotti

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…

High Energy Astrophysical Phenomena · Physics 2015-05-20 D. J. Walton , J. C. Gladstone , T. P. Roberts , A. C. Fabian

We present an analysis of the ultraluminous X-ray source (ULX) population in 75 Virgo cluster late-type galaxies, including all those with a star formation rate >~ 1 M_{sun}/yr and a representative sample of the less star-forming ones. This…

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,…

Astrophysics · Physics 2009-11-11 M. G. Watson , T. P. Roberts , M. Akiyama , Y. Ueda

Ultraluminous X-ray sources (ULXs) are some of the brightest phenomena found outside of a galaxy's nucleus, and their explanation typically invokes accretion of material onto a black hole. Here, we perform the largest population study to…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Richard M. Plotkin , Elena Gallo , Brendan P. Miller , Vivienne F. Baldassare , Tommaso Treu , Jong-Hak Woo

We report the results of a study of X-ray point sources coincident with the High Velocity System (HVS) projected in front of NGC 1275. A very deep X-ray image of the core of the Perseus cluster made with the Chandra Observatory has been…

Astrophysics · Physics 2009-09-17 O. Gonzalez-Martin , A. C. Fabian , J. S. Sanders

We present the results of two Chandra observations (separated by 1 year) of the population of X-ray sources in the spiral galaxy M51 (NGC 5194 and NGC 5195). 113 X-ray sources have been detected in an 8'.4x8'.4 region. Nine and 28 sources…

Astrophysics · Physics 2009-11-07 Yuichi Terashima , Andrew S. Wilson

We analyse all the available Chandra observations of the Cartwheel Galaxy and its compact group, taken between 2001 and 2008, with the main aim of addressing the variability in the X-ray band for this spectacular collisional ring galaxy. We…

High Energy Astrophysical Phenomena · Physics 2023-04-05 Chiara Salvaggio , Anna Wolter , Andrea Belfiore , Monica Colpi

Constraining the astrophysical nature of Ultra-Luminous X-ray (ULX) sources, which have X-ray luminosities exceeding 10^39 erg/s, has been elusive due to the optical faintness of any counterparts. With high spectral resolution observations…

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…

Astrophysics · Physics 2009-11-10 Ji-Feng Liu Joel N. Bregman , Patrick Seitzer

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…

Astrophysics · Physics 2009-11-13 Margarita Rosado , Kajal K. Ghosh , Isaura Fuentes-Carrera

Utilising archival Chandra X-ray Observatory data and Hubble Space Telescope globular cluster catalogues, we probe the time-domain properties of the low mass X-ray binary population in the elliptical galaxy NGC 4261. Of the 98 unique X-ray…

High Energy Astrophysical Phenomena · Physics 2023-07-12 Sneha Nair , Kristen Dage , Daryl Haggard , Arunav Kundu , Richard M. Plotkin , Katherine L. Rhode , Stephen E. Zepf

We present 26 point-sources discovered with Chandra within 200" (~20kpc) of the center of the barred supergiant galaxy NGC 1365. The majority of these sources are high-mass X-ray binaries, containing a neutron star or a black hole accreting…

Astrophysics · Physics 2011-02-11 Iskra V. Strateva , Stefanie Komossa

We have used XMM-Newton's Optical Monitor (OM) images to study the local environment of a sample of 27 Ultraluminous X-ray Sources (ULXs) in nearby galaxies. UVW1 fluxes were extracted from 100 pc regions centered on the ULX positions. We…

High Energy Astrophysical Phenomena · Physics 2014-03-24 Ciprian T. Berghea , Rachel P. Dudik , Jonathan Tincher , Lisa M. Winter

We report the results of a programme of dual-epoch Chandra ACIS-S observations of five ultraluminous X-ray sources (ULXs) in nearby spiral galaxies. All five ULXs are detected as unresolved, point-like X-ray sources by Chandra, though two…

Astrophysics · Physics 2009-11-10 T. P. Roberts , R. S. Warwick , M. J. Ward , M. R. Goad

The origin of Ultraluminous X-ray Sources (ULXs) in external galaxies whose X-ray luminosities exceed those of the brightest black holes in our Galaxy by hundreds and thousands of times is mysterious. The most popular models for the ULXs…

High Energy Astrophysical Phenomena · Physics 2017-02-21 S. Fabrika

We report the Chandra/ACIS-S detection of more than 20 ultraluminous X-ray sources (ULXs, L_{0.5-10 keV} >~ 3 x 10^{39} ergs/sec) in the Cartwheel collisional ring galaxy system, of which over a dozen are located in the outer active…

Astrophysics · Physics 2009-11-10 Yu Gao , Q. Daniel Wang , P. N. Appleton , Ray A. Lucas

Ultraluminous X-ray sources (ULXs) were identified as a separate class of objects in 2000 based on data from the Chandra X-Ray Observatory. These are unique objects: their X-ray luminosities exceed the Eddington limit for a typical…

Astrophysics of Galaxies · Physics 2021-05-25 S. N. Fabrika , K. E. Atapin , A. S. Vinokurov , O. N. Sholukhova