<?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%">Kontizas, M.</style></author><author><style face="normal" font="default" size="100%">Chrysovergis, M.</style></author><author><style face="normal" font="default" size="100%">Kontizas, E.</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%">Dynamical and spectral properties of some double clusters in the LMC.</style></title><short-title><style face="normal" font="default" size="100%">World of Galaxies (Le Monde des Galaxies)</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astronomical Photometry</style></keyword><keyword><style  face="normal" font="default" size="100%">Astrophysics</style></keyword><keyword><style  face="normal" font="default" size="100%">binary stars</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%">Magellanic Clouds</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds: Star Clusters</style></keyword><keyword><style  face="normal" font="default" size="100%">Spectrum Analysis</style></keyword><keyword><style  face="normal" font="default" size="100%">star clusters</style></keyword><keyword><style  face="normal" font="default" size="100%">Star Clusters: Dynamics</style></keyword><keyword><style  face="normal" font="default" size="100%">Star Clusters: Stellar Content</style></keyword><keyword><style  face="normal" font="default" size="100%">stellar evolution</style></keyword><keyword><style  face="normal" font="default" size="100%">Stellar Motions</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1989</style></year><pub-dates><date><style  face="normal" font="default" size="100%">1989/01/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1989woga.conf..145K</style></url></web-urls></urls><pages><style face="normal" font="default" size="100%">145 - 148</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">The dynamical properties and stellar content of some cluster pairs in the LMC were studied, using UKST plates. Positive evidence was found for significant distortions in the density profiles of the clusters, particularly in the outer regions. These disturbances were interpreted as indications of dynamical interaction between the pair members. Some of the pairs were found to have very similar stellar content, and ages ranging from a few 10&lt;SUP&gt;7&lt;/SUP&gt;yr to several 10&lt;SUP&gt;8&lt;/SUP&gt;yr.</style></abstract></record></records></xml>