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INTEGRAL View on cataclysmic variables and symbiotic binaries
Lutovinov A., Suleimanov V., Manuel Luna G.J., Sazonov S., Martino D.d., Ducci L., Doroshenko V., Falanga M.
© 2020 Elsevier B.V. Accreting white dwarfs (WDs) constitute a significant fraction of the hard X-ray
XSS J00564+4548 and IGR J00234+6141: New cataclysmic variables from the RXTE and INTEGRAL all-sky surveys
Bikmaev I., Revnivtsev M., Burenin R., Sunyaev R.
We present the results of our optical identification of two X-ray sources from the RXTE
Efficiency of soft X-ray radiation reprocessing in supersoft X-ray sources
Suleimanov V., Meyer F., Meyer-Hofmeister E.
We evaluate the reprocessing efficiency for soft X-rays in irradiated accretion discs of supersoft
XSS J00564+4548 and IGR J00234+6141: New cataclysmic variables from the RXTE and INTEGRAL all-sky surveys
Bikmaev I., Revnivtsev M., Burenin R., Sunyaev R.
We present the results of our optical identification of two X-ray sources from the RXTE
Statistics of white dwarf properties in intermediate polars
Suleimanov V.F., Doroshenko V.A., Werner K.
© The Author(s), 2020. Many intermediate polars are hard X-ray sources. The theory of their hard X-ray
Efficiency of soft X-ray radiation reprocessing in supersoft X-ray sources
Suleimanov V., Meyer F., Meyer-Hofmeister E.
We evaluate the reprocessing efficiency for soft X-rays in irradiated accretion discs of supersoft
RXTE broadband X-ray spectra of intermediate polars and white dwarf mass estimates
Suleimanov V., Revnivtsev M., Ritter H.
We present results of an analysis of broadband X-ray spectra of 14 intermediate polars obtained
High efficiency of soft X-ray radiation reprocessing in supersoft X-ray sources due to multiple scattering
Suleimanov V., Meyer F., Meyer-Hofmeister E.
the location where the accretion stream impinges. This area is irradiated by the X-rays where it faces
X-ray Observations of Historical Classical Nova Counterparts with eROSITA Telescope Onboard the SRG Orbital Observatory during the All-Sky Survey
Galiullin I.I., Gilfanov M.R.
Abstract: The X-ray emission from the counterparts of historical classical novae (CNe) in our
RXTE broadband X-ray spectra of intermediate polars and white dwarf mass estimates
Suleimanov V., Revnivtsev M., Ritter H.
We present results of an analysis of broadband X-ray spectra of 14 intermediate polars obtained

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