... emission mechanism, the spectral and timing analysis of the X-ray emission from microquasars (signature of accreting BH), atoll- and Z-sources (signature of accreting NS), modeling of X-Ray from close binary systems performed by RXTE, Swift, INTEGRAL and ...
... I am primarily interested in calculations on emission spectra of hydrogen and helium of the nonstable objects as T Tau stars, UV Ceti stars, AGNs and quasars. ...
... V. The origin of the x-ray emission in SS 433 in a hydrodynamical model // Astronomy ... V. "The Origin of the X-ray Emission in SS433 in a Hydrodynamic Model", 1997, Astron ...
... 159, "Multi-Wavelength Continuum Emission of AGN", Geneva, Switzerland, 30 August ... Lines and the Structure of the Emission Line Region in Active Galactic Nuclei ... No.159 "Multi-Wavelength Continuum Emission of AGN, IAU Symp. 159, p.401, Kluwer ...
... M.M.Katsova, A.M.Cherepashchuk "The Quiescent X-ray Emission of X-ray Novae and the Coronal Emission of Late-Type Stars" Astronomy Reports, 2000, V.44, 804-814 = М.М.Кацова, А.М.Черепащук "Излучение корон поздних звезд и рентгеновское излучение новых в ...
... The model of the X-ray flare source agreeing with the observed value of the emission measure, includes around 8 loops lifting up to heights around $10^{11}$~cm, i.e. more than $0.2\;R_*$. ...
... The model of the X-ray flare source agreeing with the observed value of the emission measure, includes around 8 loops lifting up to heights around $10^{11}$~cm, i.e. more than $0.2\;R_*$. ...
... In addition to iron line emission, one can see the line emission related to hydrogen ... hard emission in the energy range from 3 to 70 keV, while the direct disk emission ...