Abstract Using measured radial velocity data of five double-lined spectroscopic binary systems, HD 89959, HD 143705, HD 146361, HD 165052 and HD 152248, we find corresponding orbital and spectroscopic elements via a Probabilistic Neural Network. Our numerical results are in good agreement with those obtained by others using more traditional methods.
Keywords stars: binaries: eclipsing — binaries: spectroscopic (HD 89959, HD 143705, HD 146361, HD 165052 and HD 152248)
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