A third star in the Hercules X-ray system

Details A third star in the Hercules X-ray system A third star in the Hercules X-ray system

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213l..17m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 213, Apr. 1, 1977, p. L17-L20.

Astronomy and Astrophysics

Astrophysics

26

Binary Stars, Eccentric Orbits, Pulsars, Stellar Models, X Ray Sources, Doppler Effect, Long Term Effects, Mass Transfer, Periodic Variations

Scientific paper

It is suggested that a third, light star orbiting the Her X-1/HZ Her
system in an eccentric orbit with a period of 35 days is responsible for
the 35-day cycle and may also account for the long-term HZ Her
variations. Suggestions for some specific orbits and for further
measurements to test this model are made.

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