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Related papers: The X-ray binary population in M33: II. X-ray spec…

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We present the results of a study of the variability of X-ray sources in the central 30' of the nearby Andromeda Galaxy (M31) based on XMM Performance Verification observations. Two observations of this field, with a total exposure time of…

In an analysis of XMM-Newton archival observations of the bright Local Group spiral galaxy M 31 we study the population of X-ray sources (X-ray binaries, supernova remnants) down to a 0.2-4.5 keV luminosity of 4.4E34 erg/s. EPIC hardness…

Astrophysics · Physics 2009-11-10 W. Pietsch , M. Freyberg , F. Haberl

We report the detection of six discrete, low-luminosity (Lx < 10^33 erg/s) X-ray sources, located within 12 arcsec of the center of the collapsed-core globular cluster M30 (NGC 7099), and a total of 13 sources within the half-mass radius,…

Evidence is emerging that the luminous X-ray sources in the cores of globular clusters may often consist of, or perhaps even as a class be dominated by, ultracompact (P < 1 hr) binary stars. To the two such systems already known, in NGC…

Astrophysics · Physics 2009-10-31 Eric W. Deutsch , Bruce Margon , Scott F. Anderson

We investigated the X-ray spectral properties of a collection of low-mass X-ray binaries (LMXBs) within a sample of 15 nearby early-type galaxies observed with Chandra. We find that the spectrum of the sum of the sources in a given galaxy…

Astrophysics · Physics 2009-11-07 Jimmy A. Irwin , Alex E. Athey , Joel N. Bregman

We have carried out an in-depth study of low-mass X-ray binaries (LMXBs) detected in the nearby lenticular galaxy NGC 3115, using the Megasecond Chandra X-Ray Visionary Project observation (total exposure time 1.1 Ms). In total we found 136…

Chandra has resolved the starburst nuclear region of the face-on grand-design spiral M83. Eighty-one point sources are detected above 3.5 sigma in the ACIS S3 image, and 15 of them are within the inner 16-arcsec region of the galaxy. A…

Astrophysics · Physics 2009-11-07 Roberto Soria , Kinwah Wu

We present results from a 34 ks Chandra/ACIS-S observation of the nearby (d=3.1 Mpc) lenticular galaxy NGC 5102, previously shown to have an unusually low X-ray luminosity. We detect eleven X-ray point sources within the the $D_{25}$…

Astrophysics · Physics 2009-11-11 R. P. Kraft , L. A. Nolan , T. J. Ponman , C. Jones , S. Raychaudhury

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

We present a study of X-ray source populations in M87, the cD galaxy of the Virgo cluster, using 12 archival {\it Chandra} observations with a total exposure of $\sim$680 ks spanning about a decade. A total of 346 point-like sources are…

High Energy Astrophysical Phenomena · Physics 2018-08-08 Luan Luan , Christine Jones , William R. Forman , Ákos Bogdán , Felipe Andrade-Santos , Andy D. Goulding , Ryan C. Hickox , Meicun Hou , Zhiyuan Li

Local-Group galaxies provide access to samples of X-ray source populations of whole galaxies. The XMM-Newton survey of the Small Magellanic Cloud (SMC) completely covers the bar and eastern wing with a 5.6 deg^2 area in the (0.2-12.0) keV…

High Energy Astrophysical Phenomena · Physics 2015-06-16 R. Sturm , F. Haberl , W. Pietsch , J. Ballet , D. Hatzidimitriou , D. A. H. Buckley , M. Coe , M. Ehle , M. D. Filipovic , N. La Palombara , A. Tiengo

We searched for infrared counterparts to the cluster of X-ray point sources discovered by Chandra in the Galactic Center Region (GCR). While the sources could be white dwarfs, neutron stars, or black holes accreting from stellar companions,…

Astrophysics · Physics 2016-08-30 S. Laycock , J. Grindlay , M. van den Berg , P. Zhao , J. Hong , X. Koenig , E. M. Schlegel , S. E. Persson

We have monitored the Cassiopeia dwarf galaxy (IC 10) in a series of 10 Chandra ACIS-S observations to capture its variable and transient X-ray source population, which is expected to be dominated by High Mass X-ray Binaries (HMXBs). We…

High Energy Astrophysical Phenomena · Physics 2017-02-15 Silas G. T. Laycock , Rigel Cappallo , Benjamin F. Williams , Andrea Prestwich , Breanna Binder , Dimitris M. Christodoulou

We report on the multi-year evolution of the population of X-ray sources in the nuclear region of NGC 3621 based on Chandra, XMM-Newton and Swift observations. Among these, two sources, X1 and X5, after their first detection in 2008, seem…

We present optical lightcurves of variable stars consistent with the positions of X-ray sources identified with the Chandra X-ray Observatory for the Chandra Galactic Bulge Survey. Using data from the Mosaic-II instrument on the Blanco 4m…

We have obtained three epochs of Chandra ACIS-I observations (totaling $\sim$184 ks) of the nearby spiral galaxy NGC~300 to study the logN-logS distributions of its X-ray point source population down to $\sim$2$\times$10$^{-15}$ erg…

High Energy Astrophysical Phenomena · Physics 2017-01-18 Breanna Binder , Jacob Gross , Benjamin F. Williams , Michael Eracleous , Terrance J. Gaetz , Paul P. Plucinsky , Evan D. Skillman

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 present a systematic search for variability among the ROSAT All-Sky Survey (RASS) X-ray sources. We generated lightcurves for about 30000 X-ray point sources detected sufficiently high above background. For our variability study…

Astrophysics · Physics 2009-11-07 B. Fuhrmeister , J. H. M. M. Schmitt

We have created 0.3--10 keV, 13 year, unabsorbed luminosity lightcurves for 528 X-ray sources in the central 20' of M31. We have 174 Chandra observations spaced at ~1 month intervals thanks to our transient monitoring program, deeper…

High Energy Astrophysical Phenomena · Physics 2015-06-17 R. Barnard , M. R. Garcia , F. Primini , Z. Li , F. Baganoff , S. S. Murray

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…

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