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We report the identification of a recurrent ultraluminous X-ray source (ULX), a highly absorbed X-ray source (possibly a background AGN), and a young supernova remnant near the center of the starburst galaxy M82. From a series of Chandra…

天体物理学 · 物理学 2009-11-13 A. K. H. Kong , Y. J. Yang , P. -Y. Hsieh , D. S. Y. Mak , C. S. J. Pun

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…

We present the discovery of a new type of explosive X-ray flash in Chandra images of the old elliptical galaxy M86. This unique event is characterised by the peak luminosity of 6x10^42 erg/s for the distance of M86, the presence of…

高能天体物理现象 · 物理学 2015-06-17 P. G. Jonker , A. Glennie , M. Heida , T. Maccarone , S. Hodgkin , G. Nelemans , J. C. A. Miller-Jones , M. A. P. Torres , R. Fender

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

We report on the identification of a third, new ultraluminous X-ray source (ULX) in the starburst galaxy M82. Previously, the source was observed at fluxes consistent with the high state of Galactic black hole binaries (BHBs). We observe…

高能天体物理现象 · 物理学 2010-05-20 Jing Jin , Hua Feng , Philip Kaaret

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…

A previously undetected X-ray source (L_X<10**36 erg/s) in the strongly star-forming galaxy M83 entered an ultraluminous state between August 2009 and December 2010. It was first seen with Chandra on 23 December 2010 at L_X ~ 4 10**39…

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10$^{39}$ erg s$^{-1}$. The average number of ULXs per galaxy is still not well constrained, especially given the uncertainty on the…

This paper presents a comprehensive X-ray and multi-wavelength study of ultraluminous X-ray sources (ULXs) in NGC 1566 using archival Chandra, Swift/XRT, James Webb Space Telescope, JWST, and Hubble Space Telescope, HST observations. The…

高能天体物理现象 · 物理学 2023-11-28 Sinan Allak

We present the discovery, from archival Chandra and XMM-Newton data, of X-ray eclipses in two ultraluminous X-ray sources (ULXs), located in the same region of the galaxy M 51: CXOM51 J132940.0$+$471237 (ULX-1, for simplicity) and CXOM51…

高能天体物理现象 · 物理学 2017-02-15 Ryan Urquhart , Roberto Soria

Following a serendipitous detection with the NuSTAR observatory, we present a multi-epoch spectral and temporal analysis of an extreme ultraluminous X-ray source (ULX) located in the outskirts of the Circinus galaxy, hereafter Circinus…

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

Ultraluminous X-ray sources (ULXs) have been described variously as the most luminous normal X-ray binaries, as hypernovae, and as "intermediate-mass" black holes with masses of hundreds to thousands of solar masses. We present results on…

天体物理学 · 物理学 2009-11-11 M. I. Krauss , R. E. Kilgard , M. R. Garcia , T. P. Roberts , A. H. Prestwich

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 multi-wavelenght study of the recently discovered Ultraluminous X-ray transient XMMUJ004243.6+412519 (ULX2 hereafter) in M31, based on Swift data and the 1.8-m Copernico Telescope in Asiago (Italy). Undetected until January…

高能天体物理现象 · 物理学 2013-05-09 Fabio Pintore , Paolo Esposito , Sara Motta , Luca Zampieri

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

A new, transient ultraluminous X-ray source (ULX) was recently discovered by Chandra in M31 with a luminosity at ~ 5 x 10^39 erg/s. Here we analyse a series of five subsequent XMM-Newton observations. The steady decline in X-ray luminosity…

高能天体物理现象 · 物理学 2015-06-03 Matthew J. Middleton , Andrew D. Sutton , Timothy P. Roberts , Floyd E. Jackson , Chris Done

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

Ultra-luminous X-ray sources (ULXs) are a class of extra-galactic, point-like, off-nuclear X-ray sources with X-ray luminosity from $\sim 10^{39}$~erg s$^{-1}$ to $10^{41}$~erg s$^{-1}$. We investigated the temporal and broadband X-ray…

高能天体物理现象 · 物理学 2020-05-05 V. Jithesh , C. Anjana , Ranjeev Misra

The ultra-luminous X-ray source (ULX) M82 X-1 is one of the most promising intermediate mass black hole candidates in the local universe based on its high X-ray luminosities ($10^{40}-10^{41} {\rm erg s^{-1}}$) and quasi-periodic…

高能天体物理现象 · 物理学 2015-06-24 Xiao-jie Xu , Jifeng Liu , Jiren Liu
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