COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1643 Konkoly Observatory Budapest 1979 July 20 NEW LIGHT ELEMENTS FOR THE ECLIPSING BINARY XZ CMi Five new photoelectric minima were obtained of the short-period eclipsing variable XZ CMi during the year 1976 at the Observatory of Sierra Nevada (Granada, Spain). Times of minimum were evaluated taking on account the existence of a small asymmetry in the light curve (Breinhorst et al.). Observed values show considerable O-C's against the elements published in the "General Catalogue of Variable Stars" (I) or by Wilson (II), positive or negative respectively. min = J.D. 2428877.100 + 0.5788090d * E (I) min = J.D. 2437375.7710 + 0.57881062d * E (II) New elements were derived using our observations with linear fitting by least-squares to all available minima. As a result, a slightly shorter period was calculated and. new elements are given by, min = J.D. 2442444.4017 + 0.57880845d * E (III) O-C's corresponding to the above mentioned elements (I), (II) and (III), with the observed minimum times are the following: Minima O-C(I) O-C(II) O-C(III) p 2442444.4014 +0.018d -0.0142d -0.0003d p 2442462.3443 +0.018d -0.0144d -0.0005d p 2442463.501 +0.017d -0.015d -0.001d s 2442497.362 +0.018d -0.015d -0.001d s 2442868.380 +0.019d -0.014d +0.001d (p, indicate primary minimum and s, secondary) The plot of computed residuals from linear ephemeris for all available minima, suggests the existence of a small period change as indicated, with weaker evidences, by Wilson. A. GIMENEZ V. COSTA Instituto de Astrofisica de Andalucia Apartado 2144 Granada, Spain References: Breinhorst, R.A., Pfleiderer, J., Reinhardt, M. and Karimie, M.T.: Astron. & Astrophys. 22, 239 (1973). [BIBCODE 1973A&A....22..239B ] Wilson, R.E.: Astron. J. 71, 32 (1966). [BIBCODE 1966AJ.....71...32W ]