Optical and infrared radiation from accretion disks in be star X-ray binaries
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&#...
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| Veröffentlicht in: | Advances in space research 1988, Vol.8 (2), p.157-161 |
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| Hauptverfasser: | , , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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| Zusammenfassung: | 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. |
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| ISSN: | 0273-1177 1879-1948 |
| DOI: | 10.1016/0273-1177(88)90399-7 |