<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>5</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Cannon, R. D.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Kinematics in the Small Magellanic Cloud</style></title><short-title><style face="normal" font="default" size="100%">New Aspects of Magellanic Cloud Research</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astronomy</style></keyword><keyword><style  face="normal" font="default" size="100%">Galactic Evolution</style></keyword><keyword><style  face="normal" font="default" size="100%">Galactic Structure</style></keyword><keyword><style  face="normal" font="default" size="100%">Gravitational Effects</style></keyword><keyword><style  face="normal" font="default" size="100%">Interacting Galaxies</style></keyword><keyword><style  face="normal" font="default" size="100%">Kinematics</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds</style></keyword><keyword><style  face="normal" font="default" size="100%">Star Distribution</style></keyword><keyword><style  face="normal" font="default" size="100%">Stellar Motions</style></keyword><keyword><style  face="normal" font="default" size="100%">Stellar Systems</style></keyword><keyword><style  face="normal" font="default" size="100%">Tidal Waves</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1993</style></year><pub-dates><date><style  face="normal" font="default" size="100%">1993/01/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1993LNP...416...17H</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">416</style></volume><pages><style face="normal" font="default" size="100%">17</style></pages><isbn><style face="normal" font="default" size="100%">0075-8450</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">During the last decade several authors have undertaken extensive studies of the kinematics and structure of the Small Magellanic Cloud (SMC), which is generally thought to be affected by the dynamics of the triple interacting system consisting of the Galaxy and the Magellanic Clouds (MCs). In this paper we point out the importance of studying the kinematics of old rather than young populations when investigating the purely gravitational effects on the structure of the SMC of the previously mentioned tidal interaction. We also describe briefly the results obtained for such old stars in the NE 'corner'of the SMC.</style></abstract></record></records></xml>