Low-mass X-ray binaries
The secondary stars in cataclysmic variables and low-mass X-ray binaries
... and low-mass X-ray binaries (LMXBs), using the new catalogue of Ritter & Kolb as a starting ...reliable mass determinations of CV secondary stars (10 and 5, respectively, in the ...
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Bowen blend echo‐tomography of low mass X‐ray binaries
... Keywords: X-rays: binaries – stars: individual: Sco X-1 – stars: individual: V801 Ara PACS: ...INTRODUCTION Low mass X-ray binaries (LMXBs) are interacting ...
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Zhang, Zhongli (2012): Study of populations of low-mass X-ray binaries in elliptical galaxies. Dissertation, LMU München: Fakultät für Physik
... of low-mass X-ray binaries – dynamically formed systems in globular clusters and in the nucleus of M31, and presumably pri- mordial X-ray binaries in the fields of ...
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Voss, Rasmus (2007): Populations of low mass X-ray binaries in the galaxies Centaurus A and Andromeda. Dissertation, LMU München: Fakultät für Physik
... (L X > 10 36 erg s −1 ) X-ray point sources in the bulge of M31 is investigated using archival Chandra ...of X-ray sources, per unit stellar mass, within 1 arcmin from the centre ...
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Population synthesis of classical low-mass X-ray binaries in the Galactic Bulge
... For the subsequent evolution of the selected systems we use the LMXB tracks described in van der Sluys et al. (2005), a se- lection of which is shown in Fig. 1. These tracks describe the evolution of binaries ...
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Low-mass X-ray binaries from black hole retaining globular clusters
... as low as ...BH–BH binaries that merge in-cluster are a consequence of the large ec- centricities, acquired through dynamical formation, leading to sig- nificantly shortened orbital decay ...BH–BH ...
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An X‐Ray Variable Millisecond Pulsar in the Globular Cluster 47 Tucanae: Closing the Link to Low‐Mass X‐Ray Binaries
... peculiar X-ray spectral variability in the binary radio millisecond pulsar PSR J00247204W in the globular cluster 47 ...nonthermal X-rays originate in a relativistic intrabinary shock, formed due to ...
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A Brief Review for Quasi Periodic Oscillations in Neutron Star Low Mass X Ray Binaries
... of X-ray flux at the predicted frequencies, the reasons for variation of 𝜐𝜐 2 with luminosity, and the correlation with burst oscillations are still open ...
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The X-ray luminosity functions of field low-mass X-ray binaries in early-type galaxies : evidence for a stellar age dependence.
... 35 X-ray sources artificially added to the original FB ...one X-ray source implanted in each mock image, so that the confusion properties would not be changed by the addition of ...each ...
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Low-Mass X-ray Binaries and Globular Clusters in Early-Type Galaxies. I. Chandra Observations
... and X-ray images of the galaxy had clearly- defined centroids, we constrained the transformation to ensure approximately the same matching precision be- tween them as between GCs and ...
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Constraining the formation of black holes in short-period black hole low-mass X-ray binaries
... undergoes mass transfer within the MS- ...BH+MS-star binaries which would evolve to longer and longer periods due to the nuclear expansion of the companion, fi- nally evolving into BH+WD ...
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X-ray binary luminosity function scaling relations in elliptical galaxies : evidence for globular cluster seeding of low-mass x-ray binaries in galactic fields.
... investigate X-ray binary (XRB) luminosity function (XLF) scaling relations for Chandra-detected populations of low-mass XRBs (LMXBs) within the footprints of 24 early-type ...classify ...
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Spectral and Timing properties of Neutron Star Low-Mass X-ray Binaries. Andrea Sanna. University of Cagliari. in collaboration with:
... Scorpius X-1, we constructed its power-density spectra (van der Klis 1989) in the frequency range ...the low- and high- frequency flux variability were investigated in the bands ...
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Faint galactic X ray binaries
... Galactic X–ray ...of low–mass X–ray binaries it has recently been realised that besides a phase of radius expansion, the duration of type I X–ray bursts can ...
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Accretion in supergiant High Mass X-ray Binaries
... the X M M − Newton and INT EGRAL observations, we [12, MW11] suggested that the wind terminal velocity of the system is relatively, low, of the order of υ ∞ ∼ 500 km s −1 ...
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An X-ray, optical and infra-red study of high-mass X-ray binaries in the Small Magellanic Cloud
... with an unusual triple structure; this shape is representative of all of the other pro- files until the last few observations of the outburst. The profile in the lower panel shows how the emission geometry had changed ...
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Heating and ionization of the primordial intergalactic medium by high mass x ray binaries
... hard X-ray photons, via high energy cascades, may have deposited heat and ionizing energy into the environment in addition to that seen in the models as presented ...very low optical depths in the ...
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Obscured High Mass X-Ray Binaries and Supergiant Fast X-ray Transients: Infrared Observations of INTEGRAL Sources
... Fast X-ray Transients SFXTs constitute a new class of sources identified among the recently discovered INTE- GRAL sources, exhibiting these common characteristics: rapid outbursts lasting only hours, a ...
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Studies of the origin of high-frequency quasi-periodic oscillations of mass-accreting black holes in X-ray binaries with next-generation X-Ray telescopes
... accretion disk with a realistic power spectral density (Figure 16, top panel ). We then used the methods of Ingram & van der Klis ( 2013 ) to simulate QPOs based on the phase-resolved HS intensity from Figure 6. ...
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Fermi satellite observations of gamma-ray counterparts to radio and x-ray binaries
... States X-ray black hole binaries have, historically, shown two distinct states: the high/soft state when the source X-ray intensity is high, and the low/hard state when the ...
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