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Hercules X-1




Artist's impression of Her X-1. Credit: D. Klochkov
An X-ray pulsar that is a member of an eclipsing binary system with an orbital period of 1.7 days; it lies about 15,000 light-years away in the constellation Hercules. The visible component has been identified as the blue variable HZ Herculis, whose spectrum varies from late A or early F to B. Her X-l has a pulsation period of 1.2378 seconds, presumed to be its rotation period, and shows a 35-day quasi-periodicity in the X-ray region (but not in the optical). It is thought to move in a nearly circular orbit, to be accreting matter from HZ Her, and to have a mass of about 0.7 solar mass. The orbital period is stable, but the pulsation period is speeding up at a rate of about 1 part in 100,000 per year. The X-ray eclipse lasts 0.24 days.


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