<?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%">Zola, S.</style></author><author><style face="normal" font="default" size="100%">Rucinski, S. M.</style></author><author><style face="normal" font="default" size="100%">Baran, A.</style></author><author><style face="normal" font="default" size="100%">Ogloza, W.</style></author><author><style face="normal" font="default" size="100%">Pych, W.</style></author><author><style face="normal" font="default" size="100%">Kreiner, J. M.</style></author><author><style face="normal" font="default" size="100%">Stachowski, G.</style></author><author><style face="normal" font="default" size="100%">Gazeas, K.</style></author><author><style face="normal" font="default" size="100%">Niarchos, P.</style></author><author><style face="normal" font="default" size="100%">Siwak, M.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Physical Parameters of Components in Close Binary Systems: III</style></title><short-title><style face="normal" font="default" size="100%">Acta Astronomica</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">binaries: close</style></keyword><keyword><style  face="normal" font="default" size="100%">binaries: eclipsing</style></keyword><keyword><style  face="normal" font="default" size="100%">stars: fundamental parameters</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%">2004/09/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2004AcA....54..299Z</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">54</style></volume><pages><style face="normal" font="default" size="100%">299 - 312</style></pages><isbn><style face="normal" font="default" size="100%">0001-5237</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">The paper presents combined spectroscopic and photometric orbital solutions for five close binary systems: V 402Aur, SX Crv, V829 Her, VZ Lib and V753 Mon. The photometric data consist of new complete, multicolor light curves, while the spectroscopy has been recently obtained within the radial velocity program at the David Dunlap Observatory. For one target, SX Crv, new spectroscopic data were obtained using the 6.5 m Magellan telescope. A contact configuration was found through light curve modeling for all targets except V753 Mon. Our solution for V753 Mon resulted in a semidetached configuration with the slightly less massive component filling its Roche lobe.</style></abstract></record></records></xml>