X-Ray binaries are gravitationally bound systems consisting of a compact object that accretes matter from a companion star; they are the most interesting objects of the sky, infact they allow to study the physics of matter in very extreme conditions of density, temperature or magnetic eld. So the determination of spectral and temporal properties of X-ray binaries plays an important role in understanding the processes involved in these systems. This project aims to understand the properties of binary systems, at high inclination (dipping and eclips- ing sources), containing neutron stars weakly magnetized. In the light curves of these systems it is possible to identify a variety of modulations with orbital periodicity that are cause...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
The detection of coherent X-ray pulsations at similar to 314 Hz (3.2 ms) classifies MAXI J1957+032 a...
Satellite X-ray experiments and ground-based programs aimed at observation of X-ray binaries are dis...
X-Ray binaries are gravitationally bound systems consisting of a compact object that accretes matter...
More than half a decade of X-ray astronomy with various balloon borne and space orbiting X-ray instr...
A brief overview is given of the observations of accretion disks in X-ray binaries, discussing their...
International audienceContext. The dipping source XB 1916-053 is a compact binary system with an orb...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2011.Cataloged from PDF ve...
This work is intended to provide an introduction to multiwavelength observations of low-mass X-ray b...
1RXS J180408.9–342058 is a transient neutron star low-mass X-ray binary that exhibited a bright accr...
Context. 4U 1538−52, an absorbed high mass X-ray binary with an orbital period of ~3.73 days, shows ...
Low-mass X-ray binaries (LMXBs) are bright X-ray sources that consist of a compact object (neutron s...
MXB 1659-298 is a transient neutron-star low-mass X-ray binary system that shows eclipses with a per...
We present simultaneous high-resolution optical spectroscopy and X-ray data of the X-ray binary syst...
In all areas of astronomy a multi-wavelength approach is crucial, the work presented here demonstrat...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
The detection of coherent X-ray pulsations at similar to 314 Hz (3.2 ms) classifies MAXI J1957+032 a...
Satellite X-ray experiments and ground-based programs aimed at observation of X-ray binaries are dis...
X-Ray binaries are gravitationally bound systems consisting of a compact object that accretes matter...
More than half a decade of X-ray astronomy with various balloon borne and space orbiting X-ray instr...
A brief overview is given of the observations of accretion disks in X-ray binaries, discussing their...
International audienceContext. The dipping source XB 1916-053 is a compact binary system with an orb...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2011.Cataloged from PDF ve...
This work is intended to provide an introduction to multiwavelength observations of low-mass X-ray b...
1RXS J180408.9–342058 is a transient neutron star low-mass X-ray binary that exhibited a bright accr...
Context. 4U 1538−52, an absorbed high mass X-ray binary with an orbital period of ~3.73 days, shows ...
Low-mass X-ray binaries (LMXBs) are bright X-ray sources that consist of a compact object (neutron s...
MXB 1659-298 is a transient neutron-star low-mass X-ray binary system that shows eclipses with a per...
We present simultaneous high-resolution optical spectroscopy and X-ray data of the X-ray binary syst...
In all areas of astronomy a multi-wavelength approach is crucial, the work presented here demonstrat...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
The detection of coherent X-ray pulsations at similar to 314 Hz (3.2 ms) classifies MAXI J1957+032 a...
Satellite X-ray experiments and ground-based programs aimed at observation of X-ray binaries are dis...