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Related papers: X-ray binaries in Sculptor

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We present a comprehensive X-ray point source catalog of NGC 404 obtained as part of the Chandra Local Volume Survey. A new, 97 ks Chandra ACIS-S observation of NGC 404 was combined with archival observations for a total exposure of ~123…

High Energy Astrophysical Phenomena · Physics 2015-06-12 B. Binder , B. F. Williams , M. Eracleous , T. J. Gaetz , A. K. H. Kong , E. D. Skillman , D. R. Weisz

The twelve bright (Lx>10(36) erg/s) X-ray sources in the globular clusters have lower luminosities than the brightest sources in the bulge of our galaxy. The dim (Lx<10(35) erg/s) X-ray sources in globular clusters reach higher luminosities…

Astrophysics · Physics 2007-05-23 Frank Verbunt

We analyze 18 sources that were found to show interesting properties of periodicity, very soft spectra and/or large long-term variability in X-rays in our project of classification of sources from the 2XMMi-DR3 catalog but were poorly…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Dacheng Lin , Natalie A. Webb , Didier Barret

Current X-ray observatories make it possible to follow the evolution of transient and variable X-ray binaries across a broad range in luminosity and source behavior. In such studies, it can be unclear whether evolution in the low energy…

High Energy Astrophysical Phenomena · Physics 2014-11-20 J. M. Miller , E. M. Cackett , R. C. Reis

We present a source catalog from the first deep hard X-ray ($E>10$ keV) survey of the Small Magellanic Cloud (SMC), the NuSTAR Legacy Survey of the SMC. We observed three fields, for a total exposure time of 1 Ms, along the bar of this…

We present results of a Chandra survey of the ultra-luminous X-ray sources (ULX) in 13 normal galaxies, in which we combine source detection with X-ray flux measurement. 22 ULX were detected, i.e. with L_x > 1 x 10^{39} erg s^{-1} (L_10),…

Astrophysics · Physics 2009-09-29 P. J. Humphrey , G. Fabbiano , M. Elvis , M. J. Church , M. Balucinska-Church

We searched optical/UV/IR counterparts of seven supersoft X-ray sources (SSS) in M31 in the Hubble Space Telescope (HST) "Panchromatic Hubble Andromeda Treasury" (PHAT) archival images and photometric catalog. Three of the SSS were…

Solar and Stellar Astrophysics · Physics 2015-06-19 E. Chiosi , M. Orio , F. Bernardini , M. Henze , N. Jamialiahmadi

We investigated for a possible connection between the types of X-ray binaries (XRBs) and the properties of compact star clusters in the nearby galaxy NGC 628. Using {\it Chandra} archival data covering the years 2001-2018, 75 X-ray sources…

High Energy Astrophysical Phenomena · Physics 2023-01-25 Senay Avdan , Aysun Akyuz , Seda Acar , Inci Akkaya Oralhan , Sinan Allak , Nazim Aksaker

We report the X-ray data analysis of two transient ultraluminous X-ray sources (ULXs, hereafter X1 and X2) located in the nearby galaxy NGC 7090. While they were not detected in the 2004 XMM-Newton and 2005 Chandra observations, their…

High Energy Astrophysical Phenomena · Physics 2019-05-08 Zhu Liu , P. T. O'Brien , J. P. Osborne , P. A. Evans , K. L. Page

The rapid variability of X-ray binaries produces a wide range of X-ray states that are linked to activity across the electromagnetic spectrum. It is particularly challenging to study a sample of sources large enough to include all types in…

High Energy Astrophysical Phenomena · Physics 2023-06-30 John M. Dickey , S. D. Vrtilek , Michael McCollough , Bram Boroson , John A. Tomsick , Charles Bailyn , Jay M. Blanchard , Charlotte Johnson

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

Chandra observations of 17 nearby galaxies were analysed and 166 bright sources with X-ray counts > 100, were chosen for temporal analysis. Fractional root mean square variability amplitudes were estimated for lightcurves binned at ~ 4 ksec…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Soma Mandal , Ranjeev Misra , Gulab Dewangan

Six x-ray point sources, with luminosities of $4 \times 10^{38} - 2 \times 10^{39} \rm ergs s^{-1}$ in the 0.4--7 keV band, were detected in Chandra observations of the spiral galaxy M100. One source is identified with supernova SN 1979C…

Astrophysics · Physics 2009-11-06 Philip Kaaret

With a Chandra ACIS-S3 observation, we detect 42 X-ray point sources in the elliptical galaxy NGC 720, including a possible central source. Most of these sources will be low-mass X-ray binaries (LMXBs), and 12 are located within 2" of…

Astrophysics · Physics 2009-11-07 Tesla E. Jeltema , Claude R. Canizares , David A. Buote , Gordon P. Garmire

This paper reviews some of the recent observational results on stellar mass black hole candidates. Over the last decade, much of the progress in this field has been achieved through the study of transient X--ray binary sources which shine…

Astrophysics · Physics 2009-09-25 L. Stella , G. L. Israel , S. Mereghetti , D. Ricci

In an XMM-Newton raster observation of the bright local group spiral galaxy M33 we study the population of X-ray sources (X-ray binaries, supernova remnants, super-shells) down to a 0.5-10 keV luminosity of 10^35 erg s^-1 -- more than a…

Astrophysics · Physics 2015-06-24 W. Pietsch , M. Ehle , F. Haberl , Z. Misanovic , G. Trinchieri

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 here the results of spectral imaging observations with the ROSAT PSPC of the field surrounding the very nearby (D=3.38 Mpc) Sculptor galaxy, NGC7793. Many point sources are detected within the field, several of them showing…

Astrophysics · Physics 2007-05-23 A. M. Read , W. Pietsch

Globular clusters host a variety of lower-luminosity ($L_X<10^{35}$ erg s$^{-1}$) X-ray sources, including accreting neutron stars and black holes, millisecond pulsars, cataclysmic variables, and chromospherically active binaries. In this…

Various arguments strongly suggest that the population of ultraluminous X-ray sources (ULXs: apparent X-ray luminosity > Eddington limit for 10 Msun ~10^39 erg/s) in nearby galaxies are mostly stellar-mass X-ray binaries in unusual…

Astrophysics · Physics 2009-11-10 Andrew R. King , Walter Dehnen
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