<?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%">Gardiner, L. T.</style></author><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%">The geometry of the SMC.</style></title><short-title><style face="normal" font="default" size="100%">Proceedings of the Astronomical Society of Australia</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Astronomy</style></keyword><keyword><style  face="normal" font="default" size="100%">Color-Magnitude Diagram</style></keyword><keyword><style  face="normal" font="default" size="100%">Galactic Structure</style></keyword><keyword><style  face="normal" font="default" size="100%">Gravitational Fields</style></keyword><keyword><style  face="normal" font="default" size="100%">Luminosity</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds</style></keyword><keyword><style  face="normal" font="default" size="100%">Spatial distribution</style></keyword><keyword><style  face="normal" font="default" size="100%">Star Distribution</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1991</style></year><pub-dates><date><style  face="normal" font="default" size="100%">1991/01/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1991PASAu...9...80G</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">9</style></volume><pages><style face="normal" font="default" size="100%">80</style></pages><isbn><style face="normal" font="default" size="100%">0066-99971323-3580</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">A study is undertaken of the 3D spatial distribution of the older stellar population lying beyond about 2 kpc in projected radial distance from the center of the SMC. The study is intended to cover 120 square degrees including six overlapping Schmidt fields. The results from an area of 80 square degrees are presented including the western, northern and northeastern outer parts of the SMC.</style></abstract></record></records></xml>