<?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%">Bhatia, R. K.</style></author><author><style face="normal" font="default" size="100%">Cannon, R. D.</style></author><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">CCD observations of binary clusters in the Magellanic Clouds.</style></title><short-title><style face="normal" font="default" size="100%">European Southern Observatory Conference and Workshop Proceedings</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds:Star Clusters</style></keyword><keyword><style  face="normal" font="default" size="100%">Star Clusters:Interactions</style></keyword><keyword><style  face="normal" font="default" size="100%">Star Clusters:Magellanic Clouds</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%">1987/01/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1987ESOC...27..489B</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">27</style></volume><pages><style face="normal" font="default" size="100%">489 - 490</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">The existence of binary clusters in the Large Magellanic Cloud has been discussed recently. A survey of the LMC on UKSTU plates yielded a total of 69 pairs of clusters with a center-to-centre separation of less than ≡18 pc (for a distance modulus of 18.4 for the LMC). Statistical arguments suggest that taking chance line-ups into account, a significant fraction of the pairs found must be physically associated at the 7σ level. A series of observations have been undertaken in order to establish the physical association of the pairs.</style></abstract></record></records></xml>