<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Niarchos, P. G.</style></author><author><style face="normal" font="default" size="100%">Gazeas, K. D.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">A CCD Photometric Study of the Near-Contact System OT CEP</style></title><short-title><style face="normal" font="default" size="100%">Baltic Astronomy</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Stars: binaries: eclipsing</style></keyword><keyword><style  face="normal" font="default" size="100%">stars: individual: OT Cep</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2004</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2004/01/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2004BaltA..13..142N</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">13</style></volume><pages><style face="normal" font="default" size="100%">142 - 144</style></pages><isbn><style face="normal" font="default" size="100%">1021-6766</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">The first l VRI CCD photometric observations of the eclipsing binary system OT Cep are presented. The new times of minima, combined with the existing ones, are used to determine a new ephemeris of the system. Our light curves are analyzed with light curve synthesis techniques to derive the first geometric and photometric elements of OT Cep. The possible evolutionary status of the system is also discussed.</style></abstract></record></records></xml>