Optical study of the X-ray binary Hercules X-1

Details Optical study of the X-ray binary Hercules X-1 Optical study of the X-ray binary Hercules X-1

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...208l..31s&link_type=abstract

Astrophysical Journal, vol. 208, Aug. 15, 1976, pt. 2, p. L31-L34. NASA-supported research.

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Light Curve, Pulsars, Stellar Spectrophotometry, Ubv Spectra, X Ray Stars, Stellar Luminosity, Visual Observation

Scientific paper

The 1.7 day B-V light curve of HZ Herculis shows the existence of a
small hot component which is present only during the X-ray active
portion of the 35-day cycle. This hot component is associated with the
X-ray source since it is absent during X-ray eclipse.

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