Long time-scale variability of X-ray binaries with late-type giant companions
In this paper we propose and examine a physical mechanism which can lead to the generation of noise in themass accretion rate of low-mass X-ray binaries on time-scales comparable to the orbital period of the system.We consider modulations of mass captured
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Filippova_Long_time-scale_variability_of_2014.pdf||1.54 MB||Adobe PDF||Request a copy|
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