A method for modeling the formation of Call lines in the spectra of irradiated stellar atmospheres to calculate
model irradiated
atmospheres in a semi-grey approximation has been improved. We have modified
Accretion heated atmospheres of X-ray bursting neutron stars is well described by the
atmosphere model of a passively cooling neutron star when the burst luminosity
Radiative properties of magnetic neutron stars with metallic surfaces and thin atmospheresContext. Simple
models fail to describe the observed spectra of X-ray-dim isolated neutron stars
Investigation of Cyg OB2 #11(O5 Ifc) by modelling its atmosphere-resolution spectra. In this paper we present results of the
modelling of the stellar
atmosphere of Cyg OB2 #11
Model atmospheres of x-ray bursting neutron starsWe present an extended set of
model atmospheres and emergent spectra of X-ray bursting neutron
Models of neutron star atmospheres enriched with nuclear burning ashes the metal enrichment can change these factors. Methods. We have developed a new NS
atmosphere modeling code
35 P 09 Non linear effects of spaced distribution of aerosols in turbulent atmosphere35 P 09 Non linear effects of spaced distribution of aerosols in turbulent
atmosphere