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Related papers: Compact Stellar X-ray Sources in Normal Galaxies

200 papers

As part of our campaign to determine the nature of the various source populations of the low-luminosity globular cluster X-ray sources, we have obtained a Chandra X-ray Observatory ACIS-S3 image of the globular cluster NGC 6440. We detect…

A simple, physically consistent model has been proposed that seeks to explain in a unified way the X-ray spectra and rapid X-ray variability of the so-called Z sources and other accreting neutron stars in low-mass systems. Here we summarize…

Astrophysics · Physics 2009-10-28 Dimitrios Psaltis , Frederick K. Lamb , Guy S. Miller

Using the Chandra ACIS-I instruments, we have carried out a deep X-ray observation on the Galactic plane region at (l,b) ~ (28.5, 0.0), where no discrete X-ray sources have been known previously. We have detected, as well as strong diffuse…

{\it Chandra} Galactic Center Survey detected $\sim 800$ X-ray point-like sources in the $2^{\circ} \times 0.8^{\circ}$ sky region around the Galactic Center. In this paper, we study the spatial and luminosity distributions of these sources…

Astrophysics · Physics 2014-10-13 J. F. Wu , S. N. Zhang , F. J. Lu , Y. K. Jin

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…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Andrew D. Sutton , Timothy P. Roberts , Dominic J. Walton

We measured the X-ray fluxes from an optically-selected sample of blue compact dwarf galaxies (BCDs) with metallicities <0.07 and solar distances less than 15 Mpc. Four X-ray point sources were observed in three galaxies, with five galaxies…

Astrophysics of Galaxies · Physics 2015-05-30 Philip Kaaret , Joseph Schmitt , Mark Gorski

The dynamical production of low-mass X-ray binaries and brighter cataclysmic variables (CVs) in dense globular clusters is well-established. We investigate how the X-ray emissivity of fainter X-ray binaries (principally CVs and coronally…

X-ray observations of galaxy clusters potentially provide powerful cosmological probes if systematics due to our incomplete knowledge of the intracluster medium (ICM) physics are understood and controlled. In this paper, we study the…

Astrophysics · Physics 2015-06-24 Daisuke Nagai , Andrey V. Kravtsov , Alexey Vikhlinin

Context. The XMM-XXL survey uses observations from XMM-Newton to detect clusters of galaxies over a wide range in mass and redshift. The moderate PSF of XMM-Newton means that point sources within or projected onto a cluster may not be…

Little is presently known about the nature of ultraluminous X-ray sources (ULX). Different hypotheses have been proposed to explain their properties: intermediate-mass BHs, Kerr BHs, young SNR, or background AGN. Some of the current…

Across the Galactic disk lies a diverse population of X-ray sources, with the fainter end remaining poorly understood due to past survey sensitivity limits. We aim to classify and characterize faint X-ray sources detected in the eROSITA…

High Energy Astrophysical Phenomena · Physics 2026-01-14 Tong Bao , Gabriele Ponti , Frank Haberl , Samaresh Mondal , Mark R. Morris , Kaya Mori , Shifra Mandel , Xiao-jie Xu

Galaxies are key objects for the study of cosmology, the life cycle of matter, and stellar evolution. X-ray observations have given us a new key window into these building blocks of the Universe, that allows us to investigate their hot…

Astrophysics · Physics 2007-05-23 G. Fabbiano

Assuming that soft X-ray sources in symbiotic stars result from strong thermonuclear runaways, and supersoft X-ray sources from weak thermonuclear runaways or steady hydrogen burning symbiotic stars, we investigate the Galactic soft and…

Solar and Stellar Astrophysics · Physics 2015-05-13 Chunhua Zhu , Guoliang Lu , Zhaojun Wang , Jun Zhang

A large number of X-ray sources in globular clusters of galaxies other than the Milky Way has been found with Chandra. We discuss three issues relating to these sources. The X-ray luminosity function (XLF) of the sources in globular…

Astrophysics · Physics 2009-11-10 Walter H. G. Lewin , Frank Verbunt

XMM-Newton and Chandra have ushered in a new era for the study of dwarf galaxies in the Local Group. We provide an overview of the opportunities, challenges, and some early results. The large number of background sources relative to galaxy…

Astrophysics · Physics 2009-11-11 Rosanne Di Stefano , Roberto Soria , F. A. Primini , Albert Kong

We present a brief review of Chandra X-ray Observatory observations of neutron stars. The outstanding spatial and spectral resolution of this great observatory have allowed for observations of unprecedented clarity and accuracy. Many of…

Astrophysics · Physics 2008-11-26 M. C. Weisskopf , M. Karovska , G. G. Pavlov , V. E. Zavlin , T. Clarke

A new sample of 4299 galaxies with X-ray emission was obtained in this work by cross-correlating 2XMM catalog of X-ray sources with HyperLeda database of galaxies. We analyzed distributions of optical and X-ray fluxes, redshifts and X-ray…

Cosmology and Nongalactic Astrophysics · Physics 2013-11-19 Anatoliy Tugay

One hundred fifty-four discrete non-nuclear Ultra-Luminous X-ray (ULX) sources, with intrinsic X-ray luminosities >1e39 ergs/s, are identified in 82 galaxies observed with Chandra's Advanced CCD Imaging Spectrometer. Source positions, X-ray…

Astrophysics · Physics 2009-11-10 Douglas A. Swartz , Kajal K. Ghosh , Allyn F. Tennant , Kinwah Wu

We have used the Chandra X-ray Observatory to resolve spatially and spectrally the X-ray emission from the Circinus Galaxy. We report here on the nature of the X-ray emission from the off-nuclear point sources associated with the disk of…

Astrophysics · Physics 2009-11-06 F. E. Bauer , W. N. Brandt , R. M. Sambruna , G. Chartas , G. P. Garmire , S. Kaspi , H. Netzer

We present the source catalog of a new Chandra ACIS-I observation of NGC 300 obtained as part of the Chandra Local Volume Survey. Our 63 ks exposure covers ~88% of the D25 isophote (R~6.3 kpc) and yields a catalog of 95 X-ray point sources…