Example orbital solutions for SB2 systems with differing numbers of observed spectra and fairly good phase coverage. Black lines depict the orbital solutions, while blue and red dots represent orbital phases of the observed spectra for the primary and secondary components, respectively. V436 Per, α CrB, and NY Cep are highly eccentric binary systems with eccentricities of about 0.37, 0.38, and 0.44, respectively. RX Dra represents the case of a circular-orbit system with the previously undetected secondary component that is revealed by this work.