  Using measured radial velocity data of nine double lined spectroscopic binary
systems NSV 223, AB And, V2082 Cyg, HS Her, V918 Her, BV Dra, BW Dra, V2357
Oph, and YZ Cas, we find corresponding orbital and spectroscopic elements via
the method introduced by Karami & Mohebi (2007a) and Karami & Teimoorinia
(2007). Our numerical results are in good agreement with those obtained by
others using more traditional methods.
