Add to ORKGAbstract—We describe the results of a statistical approach to analyzing the combined radial-velocity curves of X-ray binaries with OB supergiants in a Roche model, both with and without allowance for the anisotropy of the stellar wind. We present new mass estimates for the X-ray pulsars in the clos
Observations of four massive x-ray binary stars are presented, based on data accumulated between Feb...
The masses of compact objects in X-ray binaries are best constrained through dynamical measurements,...
Abstract—We interpret the observed radial-velocity curve of the optical star in the low-mass X-ray b...
Abstract. Synthesis methods for close binary systems allow one to reliably determine fundamental par...
We have obtained the first estimates of the masses of the components of the Her X-1/HZ Her X-ray bin...
Aims. We intended to measure the radial velocity curve of the supergiant companion to the eclipsing ...
Aims. We investigate the anisotropy of stellar winds in binaries to improve the models of accretion ...
Abstract—Theoretical absorption-line profiles and radial-velocity curves for tidally deformed optica...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
We study statistical properties of the Galactic population of X-ray pulsars with ages of less than 1...
We present the results of calculations of theoretical absorption-line profiles and radial-velocity c...
PSR J2032+4127 is a young and rapidly rotating pulsar on a highly eccentric orbit around the high-ma...
Abstract: The maximum mass of a neutron star (NS) is poorly defined. Theoretical attempts to define ...
We interpret the observed radial-velocity curve of the optical star in the low-mass X-ray binary 2S ...
The aim of this PhD Thesis is to characterize a representative sample of Supergiant X-ray Binaries (...
Observations of four massive x-ray binary stars are presented, based on data accumulated between Feb...
The masses of compact objects in X-ray binaries are best constrained through dynamical measurements,...
Abstract—We interpret the observed radial-velocity curve of the optical star in the low-mass X-ray b...
Abstract. Synthesis methods for close binary systems allow one to reliably determine fundamental par...
We have obtained the first estimates of the masses of the components of the Her X-1/HZ Her X-ray bin...
Aims. We intended to measure the radial velocity curve of the supergiant companion to the eclipsing ...
Aims. We investigate the anisotropy of stellar winds in binaries to improve the models of accretion ...
Abstract—Theoretical absorption-line profiles and radial-velocity curves for tidally deformed optica...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
We study statistical properties of the Galactic population of X-ray pulsars with ages of less than 1...
We present the results of calculations of theoretical absorption-line profiles and radial-velocity c...
PSR J2032+4127 is a young and rapidly rotating pulsar on a highly eccentric orbit around the high-ma...
Abstract: The maximum mass of a neutron star (NS) is poorly defined. Theoretical attempts to define ...
We interpret the observed radial-velocity curve of the optical star in the low-mass X-ray binary 2S ...
The aim of this PhD Thesis is to characterize a representative sample of Supergiant X-ray Binaries (...
Observations of four massive x-ray binary stars are presented, based on data accumulated between Feb...
The masses of compact objects in X-ray binaries are best constrained through dynamical measurements,...
Abstract—We interpret the observed radial-velocity curve of the optical star in the low-mass X-ray b...