Optical and infrared light curves of the eclipsing X-ray binary V395 Car = 2S 0921−630
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/424/1/620/3291603/mnras0424-0620.pdf
Reference18 articles.
1. THE STRUCTURE OF THE ACCRETION DISK IN THE ACCRETION DISK CORONA X-RAY BINARY 4U 1822–371 AT OPTICAL AND ULTRAVIOLET WAVELENGTHS
2. THE OPTICAL ORBITAL LIGHT CURVE OF THE LOW-MASS X-RAY BINARY V1408 AQUILAE (= 4U 1957+115)
3. The Masses and Evolutionary State of the Stars in the Dwarf Nova SS Cygni
4. Optical and X-ray observations of 2S 0921 - 630
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1. On Its Way to the Neutron Star–White Dwarf Binary Graveyard, IGR J16194−2810, A First Ascent M Giant X-Ray Binary;The Astrophysical Journal;2024-07-01
2. Evidence for mass-dependent peculiar velocities in compact object binaries: towards better constraints on natal kicks;Monthly Notices of the Royal Astronomical Society;2023-07-27
3. A different view of wind in X-ray binaries: the accretion disc corona source 2S 0921-630;Monthly Notices of the Royal Astronomical Society;2023-06-01
4. An observationally derived kick distribution for neutron stars in binary systems;Monthly Notices of the Royal Astronomical Society;2023-03-06
5. X-ray spectroscopy of the accretion disk corona source 2S 0921−630 with Suzaku archival data;Publications of the Astronomical Society of Japan;2022-11-12
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