No CrossRef data available.
Article contents
The X-Ray Sources Sco X-1 and Cyg X-2 as Binaries
Published online by Cambridge University Press: 14 August 2015
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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