Demircan, OOzdemir, SAlbayrak, BAk, HTanriver, MDegirmenci, OLErdem, ASezer, C2019-10-272019-10-2719970185-11010185-1101https://hdl.handle.net/11454/34870A physically consistent model is presented for the early-type eclipsing binary system BF Aur, based on a simultaneous solution of its light and radial velocity curves. The less massive fainter (but hotter) secondary is smaller but almost Roche lobe filling component. The system is thus not reverse-algol. The absolute parameters of the system are found to be: M-h = 3.3 M., M-c = 4.1 M., T-h = 15600 K, T-c = 15400 K, R-h = 3.9 R., R-c = 4.1 R.. More accurate radial velocity data are needed before uniqueness can be claimed for the model.eninfo:eu-repo/semantics/closedAccessbinaries-eclipsingbinaries-spectroscopicstars-fundamental parametersstars-individual (BF Aur)Article332131135WOS:A1997YF44300008Q3Q2