Abstract
ABSTRACT New orbital elements from 14 high-dispersion spectrograms are derived for this double-line binary of type F5. The orbital elements are combined with the absence of an eclipse to derive minimum masses of 0.949)'o and 0.899)' which are consistent with either the sun-Sirius massluminosity relation or Eggen's mass-luminosity relation for the Hyades. Key words: spectroscopic binary - radial velocity - orbital elements
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