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The X-Ray Sources Sco X-1 and Cyg X-2 as Binaries
Published online by Cambridge University Press: 14 August 2015
Abstract
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The analysis of photometric observations of the X-ray source Sco X-1 leads to the conclusion of the existence of a periodic component in the light variations of this source. For 1966–74, the results can be presented as
The photoelectric observations of some authors are shown in Figure 1, using the 
period. Figure 2 shows the mean light-curve of Sco X-1. The amplitude ΔB is about 
.
- Type
- Part 9 / Variable X-Ray Sources
- Information
- Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 465 - 466
- Copyright
- Copyright © Reidel 1975
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