<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>47</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Gazeas, K. D.</style></author><author><style face="normal" font="default" size="100%">Niarchos, P. G.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">The Light-Time Effect in SZ Lyn</style></title><short-title><style face="normal" font="default" size="100%">The Light-Time Effect in Astrophysics: Causes and cures of the O-C diagram</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2005</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2005/07/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2005ASPC..335..297G</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">335</style></volume><pages><style face="normal" font="default" size="100%">297</style></pages><isbn><style face="normal" font="default" size="100%">1050-3390</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">New CCD observations of the pulsating star SZ Lyn are analyzed and a new ephemeris is proposed. The photometric data collected over the last 43 years are used to determine and update the pulsational and orbital elements, based on the light-time effect detected in the O-C diagram.</style></abstract></record></records></xml>