Abstract The results of X-ray and photometric observations (1981–1987) are given for the Be star X-ray binary A 0535+26. An analysis of the photometric and X-ray data enabled us to determine the radiation of a disk of accreting matter that gradually accumulates, precipitating afterwards on the neutron star's surface. The latter causes an X-ray flare. Physical parameters of the accreting accumulating disk are determined.
Optical and infrared radiation from accretion disks in be star X-ray binaries
Advances in Space Research ; 8 , 2-3 ; 157-161
1988-01-01
5 pages
Article (Journal)
Electronic Resource
English
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