Ri. Hynes et Pfl. Maxted, A CRITIQUE OF DISENTANGLING AS A METHOD OF DERIVING SPECTROSCOPIC ORBITS, Astronomy and astrophysics, 331(1), 1998, pp. 167-170
Multiple sets of synthetic spectra of OB-binary stars are used to test
the suitability of disentangling for deriving accurate spectroscopic
orbits. Given a set of spectra with broad phase coverage and sufficien
t total integration time (almost independent of the number of spectra)
, it appears that disentangling yields accurate and reliable semi-ampl
itudes of the spectroscopic orbits (other parameters being fixed). Met
hods for estimating the uncertainties on the derived semi-amplitudes a
re investigated.