Superhumps in low-mass X-ray binaries
نویسندگان
چکیده
منابع مشابه
Superhumps in Low–Mass X–Ray Binaries
We propose a mechanism for the superhump modulations observed in optical photometry of at least two black hole X-ray transients (SXTs). As in extreme mass–ratio cataclysmic variables (CVs), superhumps are assumed to result from the presence of the 3:1 orbital resonance in the accretion disc. This causes the disc to become non–axisymmetric and precess. However the mechanism for superhump luminos...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2001
ISSN: 0035-8711,1365-2966
DOI: 10.1046/j.1365-8711.2001.04034.x