Results 1 to 10 of about 136 (115)
Wind-accreting symbiotic X-ray binaries [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 11 pages, 4 figures, accepted in ...
Lev R Yungelson +2 more
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Optical emission-line spectra of symbiotic binaries [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT Symbiotic stars are long-period interacting binaries where the compact object, most commonly a white dwarf, is embedded in the dense stellar wind of an evolved companion star. Ultraviolet and soft X-ray emission of the accretion disc and the nuclear-burning white dwarf plays a major role in shaping the ionization balance of the ...
Kuuttila, J., Gilfanov, M.
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INTEGRAL View on cataclysmic variables and symbiotic binaries [PDF]
New Astronomy Reviews, 2020 55 pages, 8 figures, 2 tables, will be published in New Astronomy ...
Alexander Lutovinov +7 more
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Evolved Stars As Donors In Symbiotic Binaries [PDF]
EAS Publications Series, 2015 This contribution is focused on the role of cool giants in symbiotic binaries. Especially, we pay attention to their mass-loss rates and the wind mass-transfer onto their compact accretors.
Skopal, A., Sekeras, M., Shagatova, N.
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The Symbiotic Binary System EG Andromedae [PDF]
International Astronomical Union Colloquium, 1987 AbstractPhotometric observations of the symbiotic star EG and confirm that the binary system is eclipsing. The epoch of primary minimum is computed. The new period 474 days instead of 470 days is estimated by a comparison of line profiles of Balmer lines taken in 1967–69 and 1982–84.
D. Chochol +3 more
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Cl Cygni — the Well Understood Symbiotic Binary ? [PDF]
International Astronomical Union Colloquium, 1988 AbstractThe observed properties of CI Cyg are reviewed. Spectroscopic and photometric changes due to orbital effects as well as intrinsic variability of the components are discussed.
J. Mikolajewska, M. Mikolajewski
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A search for rapid photometric variability in symbiotic binaries [PDF]
Monthly Notices of the Royal Astronomical Society, 2001 We report on our survey for rapid (time scale of minutes) photometric variability in symbiotic binaries. These binaries are becoming an increasingly important place to study accretion onto white dwarfs since they are candidate Type Ia supernovae progenitors.
Sokoloski, J. L. +2 more
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Geometry of the Draco C1 Symbiotic Binary [PDF]
The Astrophysical Journal Letters, 2020 Abstract Draco C1 is a known symbiotic binary star system composed of a carbon red giant and a hot, compact companion—likely a white dwarf—belonging to the Draco dwarf spheroidal galaxy. From near-infrared spectroscopic observations taken by the Apache Point Observatory Galactic Evolution Experiment (APOGEE-2), part of Sloan Digital Sky ...
Hannah M. Lewis +16 more
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The Symbiotics as Binary Stars [PDF]
International Astronomical Union Colloquium, 1982 AbstractSymbiotic stars have become an important testing ground of various theories of binary star evolution. Several physically different models can explain them, but in each case certain fairly restrictive conditions must be met, so if we manage to identify a definite object with a model, it will tell us a lot about the structure and evolutionary ...
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Symposium - International Astronomical Union, 1992 This paper briefly reviews the physical properties of symbiotic stars: long-period interacting binaries composed of a red giant primary star and a hot companion. Two types of binaries produce symbiotic optical spectra: semi-detached systems with a main sequence secondary and detached systems with a white dwarf secondary.
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