<?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%">Hatzidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Hawkins, M. R. S.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">New results on the geometrical structure of the Small Magellanic Cloud.</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%">Magellanic Clouds: Morphology</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds: Stellar Populations</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds: Structure</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..108H</style></url></web-urls></urls><pages><style face="normal" font="default" size="100%">108 - 111</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">Most studies of the morphological and structural properties of the SMC to date were based on very young and young populations essentially confined in space to the bar, arms, and wing. In this project, the authors cover a much larger area of the SMC and a much broader range in ages, with the purpose of performing a thorough study of the structure and population synthesis in the outer regions of the SMC.</style></abstract></record></records></xml>