Secular Variation and Physical Characteristics Determination of the HADS Star EH Lib

Abstract

Physical parameters of EH Lib have been determined based on observations carried out in 2015 with photometry. They have also served, along with samples from the years 1969 and 1986, to analyse the frequency content of EH Lib with Fourier Transforms. Recent CCD observations increased the times of maximum with twelve new times which helped us study the secular variation of the period with a method based on the minimization of the standard deviation of the O--C residuals. It is concluded that there may be a long-term period change.