Seventeen years of hard X-ray observations with the instruments of the INTEGRAL observatory, with a focus on the Milky Way and in particular on the Galactic Centre region, have provided a unique database for exploration of the Galactic population of low-mass X-ray binaries (LMXBs). Our understanding of the diverse energetic phenomena associated with accretion of matter onto neutron stars and black holes has greatly improved. We review the large variety of INTEGRAL based results related to LMXBs. In particular, we discuss the spatial distribution of LMXBs over the Galaxy and their X-ray luminosity function as well as various physical phenomena associated with Atoll and Z sources, bursters, symbiotic X-ray binaries, ultracompact X-ray binarie...
High-mass X-ray binaries are fundamental in the study of stellar evolution, nucleosynthesis, structu...
Aims. We model the present-day population of classical low-mass X-ray binaries (LMXBs) with neutron ...
12 pages, 7 figures, A&A in press; updated Fig 4 with an additional spectral state, typos corrected ...
A number of new X-ray sources (IGR J17091-3624, IGR/XTE J17391-3021, IGR J17464-3213 (=XTE J17464-3...
We study the population of low-mass X-ray binaries (LMXBs) in the Galactic bulge using the deep surv...
Aims. Based on the archival data from the Chandra observations of nearby galaxies, we stud...
We have derived bias-corrected X-ray luminosity functions (XLFs) of sources detected in a uniformly ...
Low-mass X-ray binaries (LMXBs) are bright X-ray sources that consist of a compact object (neutron s...
Abstract Today's sensitive X-ray observations allow the study of populations of X-ray binaries ...
Aims.We studied and compared the long-term average hard X-ray (>20 keV) spectra of a sample of twelv...
We present an investigation of the quiescent and transient X-ray binaries (XRBs) of the Galactic Cen...
We study the Log(N)-Log(S) and X-ray luminosity function in the 2-10 keV energy band, and the spatia...
All 63 discrete X-ray sources brighter than L_{\rm X} = 5x10^{36} erg/s in any of four XMM-Newton ob...
Our collaboration is responsible for the study of a sample of 72 low mass X-ray binaries (LMXRB) usi...
We present a new technique for identifying stellar mass black holes in low mass X-ray binaries (LMXB...
High-mass X-ray binaries are fundamental in the study of stellar evolution, nucleosynthesis, structu...
Aims. We model the present-day population of classical low-mass X-ray binaries (LMXBs) with neutron ...
12 pages, 7 figures, A&A in press; updated Fig 4 with an additional spectral state, typos corrected ...
A number of new X-ray sources (IGR J17091-3624, IGR/XTE J17391-3021, IGR J17464-3213 (=XTE J17464-3...
We study the population of low-mass X-ray binaries (LMXBs) in the Galactic bulge using the deep surv...
Aims. Based on the archival data from the Chandra observations of nearby galaxies, we stud...
We have derived bias-corrected X-ray luminosity functions (XLFs) of sources detected in a uniformly ...
Low-mass X-ray binaries (LMXBs) are bright X-ray sources that consist of a compact object (neutron s...
Abstract Today's sensitive X-ray observations allow the study of populations of X-ray binaries ...
Aims.We studied and compared the long-term average hard X-ray (>20 keV) spectra of a sample of twelv...
We present an investigation of the quiescent and transient X-ray binaries (XRBs) of the Galactic Cen...
We study the Log(N)-Log(S) and X-ray luminosity function in the 2-10 keV energy band, and the spatia...
All 63 discrete X-ray sources brighter than L_{\rm X} = 5x10^{36} erg/s in any of four XMM-Newton ob...
Our collaboration is responsible for the study of a sample of 72 low mass X-ray binaries (LMXRB) usi...
We present a new technique for identifying stellar mass black holes in low mass X-ray binaries (LMXB...
High-mass X-ray binaries are fundamental in the study of stellar evolution, nucleosynthesis, structu...
Aims. We model the present-day population of classical low-mass X-ray binaries (LMXBs) with neutron ...
12 pages, 7 figures, A&A in press; updated Fig 4 with an additional spectral state, typos corrected ...