<?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%">Kontizas, M.</style></author><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Bellas-Velidis, Y.</style></author><author><style face="normal" font="default" size="100%">Cannon, R. D.</style></author><author><style face="normal" font="default" size="100%">Kontizas, E.</style></author><author><style face="normal" font="default" size="100%">Dapergolas, A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Search for Mass Segregation in NGC 2098 in the Large 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%">Astronomical Photometry</style></keyword><keyword><style  face="normal" font="default" size="100%">Astronomy</style></keyword><keyword><style  face="normal" font="default" size="100%">Interacting Galaxies</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds</style></keyword><keyword><style  face="normal" font="default" size="100%">Main Sequence Stars</style></keyword><keyword><style  face="normal" font="default" size="100%">Mass Distribution</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%">Stellar Systems</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..368K</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">416</style></volume><pages><style face="normal" font="default" size="100%">368</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%">Two very young clusters in the Large Magellanic Cloud (LMC), NGC 2098 ans SL 666, were selected for the search for mass segregation. Here we present te first results for NGC 2098. The analysis is still in progress and details will be published elsewhere. The present data confirm that the brightest main sequence stars of NGC 2098 are concentrated in the central 1.5 arcmin. The question now arises whether the cluster itself is indeed extended beyond 1.5 arcmin. Extensive star counts are now being performed in all directions and at large radii around NGC 2098 to help settle this question.</style></abstract></record></records></xml>