COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1988 Konkoly Observatory Budapest 1981 July 7 HU ISSN 0374-0676 THE ORBITAL PERIOD OF THE OLD-NOVA GK Per (1901) Forty image-tube spectra of GK Per have been obtained with the Echelle spectrograph attached at the Cassegrain focus of the 182 cm reflector of the Observatory of Asiago. The spectra cover the range lambdalambda6100-7100 A with a mean dispersion of 16.1 A/mm. The main observed feature is the Halpha emission, which shows a broad and variable line profile. Radial velocity measurements of Halpha have been derived from a mean of settings on the outer edges of the emission. The standard error for each determination is of the order of 20 km/s. Using the minimum chi^2 method, our data fit an orbit having the following elements: P = 1.9020d (+-0.000043) omega = 91 (+-6)d a sin i = 2.22 (+-0.03)x10^7km gamma =+97 (+-8) km/s e = 0.44 (+-0.25) tau= 2444249.78 (+-0.002) JD where errors are given at the 1sigma level. The orbital period hat we have derived for GK Per is in agreement with those given by Kraft (1964) and Bianchini, Hamzaoglu and Sabbadin (1981) and rejects the solution suggested by Paczynski (1965) and assumed by most authors. Attention must be paid to the interpretation of the observed eccentricity and velocity amplitude. As pointed out by Smak (1970), the hot-spot can cause a distortion of the emission profile which produces spurious amplitudes and eccentricities. A. BIANCHINI F. SABBADIN E. HAMZAOGLU Asiago Astrophysical Observatory 36012 Asiago (VI), Italy References: Bianchini, A., Hamzaoglu, E. and Sabbadin, F. 1981, Astron. Astrophys. in press [BIBCODE 1981A&A....99..392B ] Kraft, R.P. 1964., Astrophys. J. 139, 457 [BIBCODE 1964ApJ...139..457K ] Paczynski, B. 1965, Acta Astron. 15, 197 [BIBCODE 1965AcA....15..197P ] Smak, J. 1970, Acta Astron. 20, 311 [BIBCODE 1970AcA....20..311S ]