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Krzeminsky’s Optical Candidate for Cen X-3
Published online by Cambridge University Press: 25 April 2016
Extract
Cen X-3 and Her X-1 are the only two X-ray binaries which are known to pulsate periodically (at 4.8s and 1.2s respectively) in the X-ray region. The latter was identified with a fourteenth magnitude light and spectrum variable HZ Her, which was subsequently found to exhibit 1.24 second optical pulsations during certain phases. The possibility that Cen X-3 may prove to be as interesting an object optically has resulted in a wide spread search for its optical counterpart.
- Type
- X-Ray Astronomy
- Information
- Publications of the Astronomical Society of Australia , Volume 2 , Issue 5 , September 1974 , pp. 289 - 290
- Copyright
- Copyright © Astronomical Society of Australia 1974
References
Strittmatter, P. A., Scott, J., Whelan, J., Wickramasinghe, D. T., and Woolf, N. J., Astron. Astrophys., 25, 275 (1973).Google Scholar
Vidal, N. V., Wickramasinghe, D. T., Peterson, B. A., and Bessell, M. S., Astrophys. J. Lett, (in press) (1974).Google Scholar