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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.
with optically thin boundary layers, Dwarf Novae (DNs) and Symbiotic Binaries (or Symbiotic Stars, Sy
Chandra discovery of luminous supersoft X-ray sources in M81
Swartz D., Ghosh K., Suleimanov V., Tennant A., Wu K.
Binaries: symbiotic
RT Crucis: A look into the X-ray emission of a peculiar symbiotic star
Ducci L., Doroshenko V., Suleimanov V., Nikołajuk M., Santangelo A., Ferrigno C.
© 2016 ESO.Symbiotic stars are a heterogeneous class of interacting binaries. Among them, RT Cru
Optical observations of 'hot' novae returning to quiescence
-period (symbiotic) binaries. The light-curves of V4743 Sgr and V2491 Cyg present clear periodic modulations. For V
Chandra discovery of luminous supersoft X-ray sources in M81
Swartz D., Ghosh K., Suleimanov V., Tennant A., Wu K.
Binaries: symbiotic
Wind-accreting symbiotic X-ray binaries
Yungelson L., Kuranov A., Postnov K.
Society. We present a new model of the population of symbiotic X-ray binaries (SyXBs) that takes
RT Crucis: A look into the X-ray emission of a peculiar symbiotic star
Ducci L., Doroshenko V., Suleimanov V., Nikołajuk M., Santangelo A., Ferrigno C.
© 2016 ESO.Symbiotic stars are a heterogeneous class of interacting binaries. Among them, RT Cru
Determining the nature of faint X-ray sources from the ASCA Galactic center survey
Lutovinov A., Revnivtsev M., Karasev D., Shimansky V., Burenin R., Bikmaev I., Vorob’ev V., Tsygankov S., Pavlinsky M.
active G star and the other may be a symbiotic star, a red giant with an accreting white dwarf. Three
SYMBIOTIC DECISION-MAKING SYSTEMS: THE INTERSECTION OF HUMAN AND ARTIFICIAL INTELLIGENCE
Khomidov Shokhrukhkhon
, based on a "symbiotic alliance" between humans and machines. The article explores the concept
Determining the nature of faint X-ray sources from the ASCA Galactic center survey
Lutovinov A., Revnivtsev M., Karasev D., Shimansky V., Burenin R., Bikmaev I., Vorob’ev V., Tsygankov S., Pavlinsky M.
active G star and the other may be a symbiotic star, a red giant with an accreting white dwarf. Three

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