Abstract
An x-ray observation of 2S 0921-630 has been made coincident with the time of optical eclipse of this 9-day binary. No significant reduction in X-ray flux is measured. This can be explained if the binary orbit is viewed almost exactly edge-on, so that the central X-ray emitting star is obscured by the accretion disk from direct view. The X-rays that are seen are scattered into the line of sight by material above and below the disk and the apparent size of the X-ray emission region is thus large compared to the size of the occulting star.
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Mason, K.O., Cordova, F.A., Corbet, R.H.D. et al. An EXOSAT observation of the peculiar X-ray binary 2S 0921-630 during optical eclipse. Space Sci Rev 40, 225–228 (1985). https://doi.org/10.1007/BF00212889
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DOI: https://doi.org/10.1007/BF00212889