2509 20160701171706.0 ASTROimport-666 Freyhammer, L. M. 2004 The eclipsing binary HD 92024: getting the orbit HD 92024 (=V381 Car) is an SB1 eclipsing binary system with a ß Cephei star as primary component. We report on the progress of a combined photometric and spectroscopic investigation of this binary, being the only one of its kind known in the southern hemisphere. Pulsating components of spectroscopic binaries often introduce substantial line-profile variations in the spectra that hamper the determination of orbital radial-velocity amplitudes, and thus also of the stellar masses. Here, in order to minimise the bias from line-profile variations on the orbital RVs, we use selected matched-profile RV differences to derive the orbital parameters. The method is compared to straightforward cross-correlation with an averaged spectrum. Hensberge, H. Sterken, C. Pavlovski, K. Smetter, A. Ilijic, S. Spectroscopically and Spatially Resolving the Components of the Close Binary Stars 318 2004 334-337 http://esoads.eso.org/abs/2004ASPC..318..334F published in NONREF