Optical variability of HZ Herculis, 1982-1983 - Normal state and anomalous 35-day behavior

Details Optical variability of HZ Herculis, 1982-1983 - Normal state and anomalous 35-day behavior Optical variability of HZ Herculis, 1982-1983 - Normal state and anomalous 35-day behavior

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..429m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, June 1984, p. 429-433) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, May-June

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Electrophotometry, Stellar Spectrophotometry, Variable Stars, Visual Photometry, X Ray Sources, Light Curve, Pulsars, Ultraviolet Spectra, X Ray Spectra

Scientific paper

Photoelectric WBVR observations of the HZ Her system have shown that the
amplitude of the "reflection effect" in 1983 was not significantly
changed despite the anomalous 35-day X-ray cycle behaviour. In the UV
range as well as in other spectral bands some differences in the shape
of the light curves are observed.

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