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Comparison of the X-Ray Sources CIR X-1. GX301-2 and 2S0535-668
Published online by Cambridge University Press: 25 April 2016
Extract
There is reasonably strong evidence to suggest that the periodic X-ray, radio and optical variable Cir X-1 is a highly eccentric orbit (e ~ 0.8), binary system comprising an OB supergiant primary and a compact object, probably a neutron star (Whelan et al. 1977; Haynes, Lerche and Murdin 1980).
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- Copyright © Astronomical Society of Australia 1980
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