Using measured radial velocity data of five double-lined spectroscopic binary systems EQ Tau, V376 And, V776 Cas, V2377 Oph and V380 Cygni, we find corresponding orbital and spectroscopic elements via the method introduced by Karami & Teimoorinia and Karami & Mohebi. Our numerical results are in good agreement with those obtained by others using more traditional methods.
Karami, K. & Mohebi, R. (2019). Velocity curve analysis of spectroscopic binary stars EQ Tau, V376 And, V776 Cas, V2377 Oph and V380 Cygni by nonlinear regression. Iranian Journal of Physics Research, 9(3), 293–293.
MLA
Karami, K., & Mohebi, R. "Velocity curve analysis of spectroscopic binary stars EQ Tau, V376 And, V776 Cas, V2377 Oph and V380 Cygni by nonlinear regression", Iranian Journal of Physics Research, 9, 3, 2019, 293–293.
HARVARD
Karami, K., & Mohebi, R. (2019). 'Velocity curve analysis of spectroscopic binary stars EQ Tau, V376 And, V776 Cas, V2377 Oph and V380 Cygni by nonlinear regression', Iranian Journal of Physics Research, 9(3), pp. 293–293.
CHICAGO
Karami, K. & Mohebi, R., "Velocity curve analysis of spectroscopic binary stars EQ Tau, V376 And, V776 Cas, V2377 Oph and V380 Cygni by nonlinear regression." Iranian Journal of Physics Research, 9 3 (2019): 293–293,
VANCOUVER
Karami K., Mohebi R. Velocity curve analysis of spectroscopic binary stars EQ Tau, V376 And, V776 Cas, V2377 Oph and V380 Cygni by nonlinear regression. Iranian Journal of Physics Research. 2019;9(3):293–293 (In Persian).
