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Related papers: X-ray binaries in M51 I: catalog and statistics

200 papers

We present an analysis of the compact X-ray source population in the Seyfert~2 galaxy NGC 1068, imaged with Chandra. We find a total of 84 compact sources, of which 66 are projected onto the galactic disk of NGC 1068. Spectra of the…

Astrophysics · Physics 2009-11-07 David A. Smith , Andrew S. Wilson

The Chandra X-ray Observatory has now discovered nearly 10,000 X-ray point sources in the 2 x 0.8 degree region around the Galactic Center (Muno 2009). The sources are likely to be a population of accreting binaries in the Galactic Center,…

We report the identification of a possible optical counterpart to the super-Eddington X-ray source NGC 5204 X-1. New Chandra data shows that the X-ray source is point-like, with a luminosity of 5.2 x 10^39 erg/s (0.5 - 8 keV). It displays…

Astrophysics · Physics 2009-11-06 T. P. Roberts , M. R. Goad , M. J. Ward , R. S. Warwick , P. T. O'Brien , P. Lira , A. D. P. Hands

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…

High Energy Astrophysical Phenomena · Physics 2015-05-27 P. H. Sell , D. Pooley , A. Zezas , S. Heinz , J. Homan , W. H. G. Lewin

Using a deep Chandra AO-1 observation of the face-on spiral galaxy M101, we examine three of five previously optically-identified X-ray sources which are spatially correlated with optical supernova remnants (MF54, MF57, and MF83). The X-ray…

Astrophysics · Physics 2009-11-06 S. L. Snowden , K. Mukai , W. Pence , K. D. Kuntz

X-ray binaries (XRBs) are probes of both star formation and stellar mass, but more importantly remain one of the only direct tracers of the compact object population. To investigate the XRB population in M31, we utilized all 121 publicly…

Astrophysics of Galaxies · Physics 2015-06-22 N. Vulic , S. C. Gallagher , P. Barmby

Based on the archival data from the Chandra observations of nearby galaxies, we study different sub populations of low-mass X-ray binaries (LMXBs) - dynamically formed systems in globular clusters (GCs) and in the nucleus of M31 and…

We present results from a 47 ks observation of the Andromeda galaxy, M31, using the High-Resolution Camera of the Chandra X-Ray Observatory. We detect 142 point sources spanning three orders of magnitude in luminosity, from $L_X = 2\times…

Astrophysics · Physics 2009-11-07 Philip Kaaret

We report on \chandra observations of the central region of M31. By combining eight \chandra ACIS-I observations taken between 1999 and 2001, we have identified 204 X-ray sources within the central $\sim 17'\times17'$ region of M31, with a…

We present X-ray and optical observations of a new transient X-ray source in M31 first detected 23-May-2004 at R.A.=00:43:09.940 +/- 0.65'', Dec.=41:23:32.49 +/- 0.66''. The X-ray lightcurve shows two peaks separated by several months,…

Ultraluminous X-Ray Objects are off-nucleus point sources 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 optical counterparts by…

Astrophysics · Physics 2009-11-07 Ji-Feng Liu , Joel N. Bregman , Patrick Seitzer

A Chandra X-Ray Observatory ACIS-S imaging observation is used to study the population of X-ray sources in the nearby Sab galaxy M81 (NGC 3031). A total of 177 sources are detected with 124 located within the D25 isophote to a limiting…

All 63 discrete X-ray sources brighter than L_{\rm X} = 5x10^{36} erg/s in any of four XMM-Newton observations of the core of M31 were surveyed for time variability over time-scales of seconds to thousands of seconds, and for intensity…

Astrophysics · Physics 2016-08-30 R. Barnard , U. Kolb , J. P. Osborne

We present Chandra X-ray Observatory ACIS-S3 X-ray imaging observations and VLT/FORS2 and Hubble Space Telescope optical observations of two low-density Galactic globular clusters; NGC 6366 and M55. We detect 16 X-ray sources with 0.5-6.0…

Astrophysics · Physics 2009-11-13 C. G. Bassa , D. Pooley , F. Verbunt , L. Homer , S. F. Anderson , W. H. G. Lewin

(Abridged) We present the results of the systematic survey of X-ray sources in the central region of M31 using the data from XMM-Newton observations performed in the years 2000-2004. The spectral properties and variability of 123 bright…

Astrophysics · Physics 2007-05-23 Sergey Trudolyubov , William Priedhorsky , France Cordova

We discovered eclipses and dips in two luminous (and highly variable) X-ray sources in M\,51. One (CXOM51 J132943.3$+$471135) is an ultraluminous supersoft source, with a thermal spectrum at a temperature of about 0.1 keV and characteristic…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Song Wang , Roberto Soria , Ryan Urquhart , Jifeng Liu

We present new optical spectroscopy of 20 candidate counterparts of 17 X-ray sources in the direction of the M31 disc. By comparing the X-ray catalogue from the XMM-Newton survey of M31 with star catalogues from the Local Group Galaxy…

We report results from Hubble Space Telescope WFPC2 imaging of the field of the luminous, bursting X-ray source in the globular cluster NGC 6441. Although the X-ray position is known to a precision of a few arcseconds, this source is only…

Astrophysics · Physics 2009-10-30 Eric W. Deutsch , Scott F. Anderson , Bruce Margon , Ronald A. Downes

We present a catalog of 5184 candidate infrared counterparts to X-ray sources detected towards the Galactic center. The X-ray sample contains 9017 point sources detected in this region by the Chandra X-ray Observatory, including data from a…

Astrophysics of Galaxies · Physics 2009-09-28 Jon C. Mauerhan , Michael P. Muno , Mark R. Morris , Franz E. Bauer , Shogo Nishiyama , Tetsuya Nagata

Building on recent work by Chandar et al. (2020), we construct X-ray luminosity functions (XLFs) for different classes of X-ray binary (XRB) donors in the nearby star-forming galaxy M83 through a novel methodology: rather than classifying…

High Energy Astrophysical Phenomena · Physics 2021-05-12 Qiana Hunt , Elena Gallo , Rupali Chandar , Paula Johns Mulia , Angus Mok , Andrea Prestwich , Shengchen Liu