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相关论文: The Luminous X-ray Source Population in M51 Observ…

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A deep (98.2 ks) Chandra Cycle-1 observation has revealed a wealth of discrete X-ray sources as well as diffuse emission in the nearby face-on spiral galaxy M101. From this rich dataset we have created a catalog of the 110 sources from the…

天体物理学 · 物理学 2009-11-06 W. D. Pence , S. L. Snowden , K. Mukai , K. D. Kuntz

(Abridged) We conducted a Chandra ACIS observation of the nearby Sculptor Group Sd galaxy NGC 7793. At the assumed distance to NGC 7793 of 3.91 Mpc, the limiting unabsorbed luminosity of the detected discrete X-ray sources (0.2-10.0 keV) is…

Recent observations of galaxies continue to reveal new ultraluminous X-ray sources (ULXs), increasing their known population and improving the statistics needed to understand their nature. We study the ULX populations of NGC 4631 and NGC…

高能天体物理现象 · 物理学 2026-03-11 Sinan Allak , Aysun Akyuz , Yasemin Aladag , Lorenzo Ducci , Andrea Santangelo

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…

天体物理学 · 物理学 2011-02-11 Iskra V. Strateva , Stefanie Komossa

We report the detailed analysis of the X-ray properties of the discrete sources detected in a long (72 ks) \chandra ACIS-S observation of the Antennae galaxies. We detect 49 sources, down to a detection limit of ~ 10^{38} erg\s; 18 sources…

天体物理学 · 物理学 2009-11-07 A. Zezas , G. Fabbiano , A. H. Rots , S. S. Murray

We present an analysis of 15 Chandra observations of the nearby spiral galaxy M81 taken over the course of six weeks in May--July 2005. Each observation reaches a sensitivity of ~10^37 erg/s. With these observations and one previous deeper…

高能天体物理现象 · 物理学 2015-05-27 P. H. Sell , D. Pooley , A. Zezas , S. Heinz , J. Homan , W. H. G. Lewin

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 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…

高能天体物理现象 · 物理学 2023-04-05 Chiara Salvaggio , Anna Wolter , Andrea Belfiore , Monica Colpi

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

VLT images in $BVI$ are used to identify the optical counterparts to bright CHANDRA X-ray points sources discovered by Kraft et al. (2001, ApJ, 560, 675) in NGC5128. Of a total of 111 X-ray point sources with L_X>2*10^{36} ergs/s present in…

天体物理学 · 物理学 2009-11-10 Dante Minniti , Marina Rejkuba , Jose G. Funes S. J. , Sanae Akiyama

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…

We use a set of conservative criteria to identify luminous supersoft X-ray sources(SSSs) in external galaxies. We test this approach on blackbody models, and then apply it to {\it Chandra} data from 4 galaxies: an elliptical (NGC 4967), 2…

天体物理学 · 物理学 2009-11-07 R. Di Stefano , A. K. H. Kong

We report on the {\it Chandra} observations of the elliptical galaxy NGC 1399, concentrating on the X-ray sources identified with globular clusters (GCs). A large fraction of the 2-10 keV X-ray emission in the $8' \times 8'$ {\it Chandra}…

天体物理学 · 物理学 2019-08-17 Lorella Angelini , Michael Loewenstein , Richard F. Mushotzky

The more than 80 nearby galaxies imaged with the Chandra Advanced CCD Imaging Spectrometer have been analyzed in a search for Ultra-Luminous X-ray (ULX) sources. The sample of galaxies span the range of Hubble morphological types and…

天体物理学 · 物理学 2007-05-23 Douglas A. Swartz , Kajal K. Ghosh , Allyn F. Tennant

We present the results of a complete spectral survey of the X-ray point sources detected in five XMM-Newton observations along the major axis of M31 but avoiding the central bulge, aimed at establishing the population characteristics of…

天体物理学 · 物理学 2009-11-13 L. Shaw Greening , R. Barnard , U. Kolb , C. Tonkin , J. P. Osborne

We present highlights from a study of a sample of 10 extreme-luminosity candidate ultraluminous X-ray sources (L_X > 5 x 10^(40) erg sec^(-1)), all at distances < 100 Mpc, identified from a cross-correlation of the RC3 catalogue of galaxies…

高能天体物理现象 · 物理学 2015-05-20 Andrew D. Sutton , Timothy P. Roberts , Dominic J. Walton

Using the Chandra Source Catalog 2.0 and a newly compiled catalogue of galaxies in the local Universe, we deliver a census of ultraluminous X-ray source (ULX) populations in nearby galaxies. We find 629 ULX candidates in 309 galaxies with…

The population of low-luminosity (< 10^35 erg/s) X-Ray Binaries (XRBs) has been investigated in our Galaxy and M31 but not further. To address this problem, we have used data from the Chandra X-Ray Observatory and the Hubble Space Telescope…

宇宙学与河外天体物理 · 物理学 2015-06-12 N. Vulic , P. Barmby , S. C. Gallagher

We present results from a Chandra study of ultraluminous X-ray sources (ULXs) in a sample of 17 nearby (D_L<60 Mpc) luminous infrared galaxies (LIRGs), selected to have star formation rates (SFRs) in excess of 7 M_sun yr^-1 and low…

高能天体物理现象 · 物理学 2015-06-23 W. Luangtip , T. P. Roberts , S. Mineo , B. D. Lehmer , D. M. Alexander , F. E. Jackson , A. D. Goulding , J. L. Fischer

This study represents the most sensitive Chandra X-ray point source catalogue of M31. Using 133 publicly available Chandra ACIS-I/S observations totalling ~1 Ms, we detected 795 X-ray sources in the bulge, northeast, and southwest fields of…

星系天体物理 · 物理学 2016-07-07 N. Vulic , S. C. Gallagher , P. Barmby