Reveals the connection between the eclipse periods of HZ Herculis and Hercules X-1, highlighting its optical characteristics.
It is shown that HZ Hercutis has an eclipse period and phase equal to the eclipse period and phase of the pulsating X-ray source Hercules X-1. Data for HZ Hercutis are also given for the light curve, colors, proper motIon, and the influence of the 35 day X-ray cycle on the optical light. A model for the binary system is described and the optical light curve is calculated.
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Bahcall et al. (1972) studied this question.
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