<?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%">Kontizas, M.</style></author><author><style face="normal" font="default" size="100%">Hadjidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Kontizas, E.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Masses and tidal radii of the star clusters in the halo of the LMC. I.</style></title><short-title><style face="normal" font="default" size="100%">Astronomy and Astrophysics Supplement Series</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astronomical Catalogs</style></keyword><keyword><style  face="normal" font="default" size="100%">Astrophysics</style></keyword><keyword><style  face="normal" font="default" size="100%">Globular Clusters</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds</style></keyword><keyword><style  face="normal" font="default" size="100%">radii</style></keyword><keyword><style  face="normal" font="default" size="100%">star clusters</style></keyword><keyword><style  face="normal" font="default" size="100%">Star Distribution</style></keyword><keyword><style  face="normal" font="default" size="100%">stellar evolution</style></keyword><keyword><style  face="normal" font="default" size="100%">Stellar Mass</style></keyword><keyword><style  face="normal" font="default" size="100%">Tides</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1987</style></year><pub-dates><date><style  face="normal" font="default" size="100%">1987/03/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1987A&amp;AS...68..493K</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">68</style></volume><pages><style face="normal" font="default" size="100%">493 - 514</style></pages><isbn><style face="normal" font="default" size="100%">0365-0138</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">An investigation of the star clusters in the outermost areas of the LMC has started in order to examine the observed dynamical properties of the halo globular clusters in this galaxy. A first sample of 38 clusters have been measured by means of star counts on plates taken with the 1.2 m U.K. Schmidt telescope. The derived tidal radii and masses are comparable to those found for the disk young clusters of the LMC and those of the galactic globulars.</style></abstract></record></records></xml>