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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 perform empirical fits to the \emph{Chandra} and \emph{XMM-Newton} spectra of three ultraluminous X-ray sources (ULXs) in the edge-on spiral galaxy NGC 891, monitoring the region over a seventeen year time window. One of these sources…

高能天体物理现象 · 物理学 2022-02-22 Nicholas M. Earley , Vikram V. Dwarkadas , Victoria Cirillo

We present a new, multi-mission catalogue of ultraluminous X-ray source (ULX) candidates, based on recent data releases from each of the XMM-Newton, Swift and Chandra observatories (the 4XMM-DR10, 2SXPS and CSC2 catalogues, respectively).…

高能天体物理现象 · 物理学 2021-10-27 D. J. Walton , A. D. A. Mackenzie , H. Gully , N. R. Patel , T. P. Roberts , H. P. Earnshaw , S. Mateos

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…

Two recent observations of the nearby galaxy NGC 6946 with NuSTAR, one simultaneous with an XMM-Newton observation, provide an opportunity to examine its population of bright accreting sources from a broadband perspective. We study the…

We report on the serendipitous discovery of a new transient in NGC 5907, at a peak luminosity of 6.4x10^{39} erg/s. The source was undetected in previous 2012 Chandra observations with a 3 sigma upper limit on the luminosity of 1.5x10^{38}…

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

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 1e39 erg/s. The ULX population counts several hundreds objects but only a minor fraction is well studied. Here we present a detailed…

A sub-set of the brightest ultraluminous X-ray sources (ULXs), with X-ray luminosities well above $10^{40}$ erg s$^{-1}$, typically have energy spectra which can be well described as hard power-laws, and short-term variability in excess of…

高能天体物理现象 · 物理学 2016-04-06 F. Pintore , L. Zampieri , A. D. Sutton , T. P. Roberts , M. J. Middleton , J. C. Gladstone

We report the discovery of a new ultraluminous X-ray source (ULX) associated with a globular cluster in the elliptical galaxy NGC 4649. The X-ray source was initially detected with a luminosity below 5 x 10^38 erg/s, but in subsequent…

We have re-examined the most luminous X-ray sources in the starburst galaxy NGC 4631, using XMM-Newton, Chandra and ROSAT data. The most interesting source is a highly variable supersoft ULX. We suggest that its bolometric luminosity ~ a…

高能天体物理现象 · 物理学 2011-02-11 Roberto Soria , Kajal Ghosh

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

We report on the discovery of a new, transient ultraluminous X-ray source (ULX) in the galaxy NGC 7090. This new ULX, which we refer to as NGC 7090 ULX3, was discovered via monitoring with $Swift$ during 2019-20, and to date has exhibited a…

Despite the 30-year history of ultra-luminous X-ray sources (ULXs) studies, issues like the majority of their physical natures (i.e., neutron stars, stellar-mass black holes, or intermediate black holes) as well as the accretion mechanisms…

高能天体物理现象 · 物理学 2023-08-15 Chen-Hsun Ma , Kwan-Lok Li , You-Hua Chu , Albert K. H. Kong

We present a multi-mission X-ray analysis of a bright (peak observed 0.3-10 keV luminosity of ~ 6x10^{40} erg s^{-1}), but relatively highly absorbed ULX in the edge-on spiral galaxy NGC 5907. The ULX is spectrally hard in X-rays (Gamma ~…

The advanced capabilities of the Chandra and XMM-Newton observatories mean that, for the first time, the detailed study of the brightest point-like X-ray sources in nearby galaxies outside of the local group is a realistic aim. Here, we…

天体物理学 · 物理学 2007-05-23 T. P. Roberts , M. R. Goad , M. J. Ward , R. S. Warwick , P. Lira

In this study, we report identification of a new ultraluminous X-ray source (ULX) named as X-7 in NGC 1316, with an unabsorbed luminosity of 2.1$\times$10$^{39}$ erg s$^{-1}$ using the two recent Chandra archival observations. The X-7 was…

高能天体物理现象 · 物理学 2020-11-05 S. Allak , A. Akyuz , N. Aksaker , M. Ozdogan Ela , S. Avdan , F. Soydugan

We present a high-quality hard X-ray spectrum of the ultraluminous X-ray source (ULX) NGC 5643 X-1 measured with NuSTAR in May-June 2014. We have obtained this spectrum by carefully separating the signals from the ULX and from the active…

高能天体物理现象 · 物理学 2016-08-31 Roman Krivonos , Sergey Sazonov

In recent work with high-resolution grating spectrometers (RGS) aboard XMM-Newton Pinto et al. (2016) have discovered that two bright and archetypal ultraluminous X-ray sources (ULXs) have strong relativistic winds in agreement with…

高能天体物理现象 · 物理学 2017-05-03 C. Pinto , W. Alston , R. Soria , M. J. Middleton , D. J. Walton , A. D. Sutton , A. C. Fabian , H. Earnshaw , R. Urquhart , E. Kara , T. P. Roberts

We report the discovery of a new candidate ultraluminous X-ray source (ULX) in the nearby edge-on spiral galaxy NGC 891. The source, which has an absorbed flux of F_X ~ 10^-12 erg/s/cm^2 (corresponding to L_X > 10^40 erg/s at 9 Mpc), must…

高能天体物理现象 · 物理学 2015-06-04 Edmund J. Hodges-Kluck , Joel N. Bregman , Jon M. Miller , Eric W. Pellegrini
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