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. and 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. , and 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
K. Karami and R. Mohebi, "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. Dear user; Recently we have changed our software to Sinaweb. If you had already registered with the old site, you may use the same USERNAME but you need to change your password. To do so at the first use, please choose, 2019; 9(3): 293-293.
