We present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron stars in low mass X-ray binaries. Compton scattering is taken into account. The models were computed in LTE approximation for six different chemical compositions: pure hydrogen and pure helium atmospheres, and atmospheres with a solar mix of hydrogen and helium and various heavy elements abundances; Z=1, 0.3, 0.1, and 0.01 Z⊙, for three values of gravity, logg=14.0, 14.3, and 14.6 and for 20 values of relative luminosity l=L/LEdd in the range 0.001-0.98. The emergent spectra of all models are fitted by diluted blackbody spectra in the observed RXTE/PCA band 3-20 keV and the corresponding values of color correction factors fc are presented. We also...
Aims. Emergent model spectra of neutron-star atmospheres are widely used to fit the observed soft X-...
Aims.Emergent model spectra of neutron-star atmospheres are widely used to fit the observed soft X-r...
Context. Low-mass X-ray binaries hosting neutron stars (NS) exhibit thermonuclear (type-I) X-ray bur...
We present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron stars...
Aims. X-ray bursting neutron stars in low-mass X-ray binaries constitute an appropriate so...
Aims. X-ray bursting neutron stars in low-mass X-ray binaries constitute an appropriate source class...
The hydrogen and helium accreted by X-ray bursting neutron stars is periodically consumed in runaway...
Some thermonuclear (type I) X-ray bursts at the neutron star surfaces in low-mass X-ray binaries tak...
Context. Theoretical spectra of X-ray bursting neutron star (NS) model atmospheres are widely used t...
© 2016, SIF, Springer-Verlag Berlin Heidelberg. Model spectra of neutron star atmospheres are nowada...
This paper presents the set of plane-parallel model atmosphere equations for a very hot neutron star...
Context. Theoretical spectra of X-ray bursting neutron star (NS) model atmospheres are wid...
Using deep Chandra observations of the globular cluster M28, we study the quiescent X-ray emission o...
Aims. Emergent model spectra of neutron-star atmospheres are widely used to fit the observed soft X-...
Aims.Emergent model spectra of neutron-star atmospheres are widely used to fit the observed soft X-r...
Context. Low-mass X-ray binaries hosting neutron stars (NS) exhibit thermonuclear (type-I) X-ray bur...
We present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron stars...
Aims. X-ray bursting neutron stars in low-mass X-ray binaries constitute an appropriate so...
Aims. X-ray bursting neutron stars in low-mass X-ray binaries constitute an appropriate source class...
The hydrogen and helium accreted by X-ray bursting neutron stars is periodically consumed in runaway...
Some thermonuclear (type I) X-ray bursts at the neutron star surfaces in low-mass X-ray binaries tak...
Context. Theoretical spectra of X-ray bursting neutron star (NS) model atmospheres are widely used t...
© 2016, SIF, Springer-Verlag Berlin Heidelberg. Model spectra of neutron star atmospheres are nowada...
This paper presents the set of plane-parallel model atmosphere equations for a very hot neutron star...
Context. Theoretical spectra of X-ray bursting neutron star (NS) model atmospheres are wid...
Using deep Chandra observations of the globular cluster M28, we study the quiescent X-ray emission o...
Aims. Emergent model spectra of neutron-star atmospheres are widely used to fit the observed soft X-...
Aims.Emergent model spectra of neutron-star atmospheres are widely used to fit the observed soft X-r...
Context. Low-mass X-ray binaries hosting neutron stars (NS) exhibit thermonuclear (type-I) X-ray bur...