UBV photometry of HZ Herculis - The shape of the primary minimum

Details UBV photometry of HZ Herculis - The shape of the primary minimum UBV photometry of HZ Herculis - The shape of the primary minimum

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....90...54k&link_type=abstract

Astronomy and Astrophysics, vol. 90, no. 1-2, Oct. 1980, p. 54-57.

Astronomy and Astrophysics

Astrophysics

15

Eclipsing Binary Stars, Electrophotometry, Ubv Spectra, X Ray Stars, Colorimetry, Light Curve, Stellar Magnitude, Stellar Models

Scientific paper

Five nights of photoelectric observations in UBV are discussed and
compared with model predictions. It is shown that a total eclipse phase
exists, which is shorter than the X-ray eclipse and that a marked
asymmetry is present near primary minimum connected with a rather hot
source of radiation.

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