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    In:  Other Sources
    Publication Date: 2011-08-16
    Description: 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.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; 208; Aug. 15
    Format: text
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