COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2092 Konkoly Observatory Budapest 1982 February 23 HU ISSN 0374-0676 SPECTROSCOPIC OBSERVATIONS OF V 471 TAURI (BD+16d516) This RS CVn type eclipsing variable was spectroscopically observed at the Astrophysical Observatory of Asiago. Continuous observations cover the period from November 1980 to February 1981. Observations were achieved with the telescopes with 122 and 182 cm diameters. The first instrument is equipped with medium dispersion prism spectrograph (40 A mm^-1 at 4340 A) and the second one with high dispersion Reosce Echelle spectrograph (16 A mm^-1 at 6563 A). 70 medium and 7 high dispersion spectra were secured with the 122 cm and 182 cm telescopes. Some of the medium dispersion spectra were obtained in a single trail mode (Walker and Chincarini, 1968). 35 spectra were utilized in the computer construction of the radial velocity curve (see Fig. 1.) and the spectroscopic orbital elements were calculated. [FIGURE 1] Fig. 1. Computer constructed radial velocity curve of V 471 Tauri The orbital elements and their probable errors can be summarized as: Elements Probable Errors V0 = 40.1 km s^-1 2.06 km s^-1 P = 0.52118286 day (assumed constant) passage from periastron = 2444970.716 0.027 day omega = 101d 18.9d e = 0.0548 0.0275 a.Sini = 1.07 x 10^6 km 2.05 x 10^4 K = 150 km s^-1 2.86 km s^-1 Note: Complete references for this star were not repeated instead they can be found in Hamzaoglu, 1981. Acknowledgements: E.H is grateful to TUBITAK for their encouragement. E. HAMZAOGLU (x) and F. SABBADIN Astrophysical Observatory of Asiago 36012 (VIC) Italy (x) Permanent address: Ege University Observatory P.K. 21 Izmir-Turkey