<?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, Despina</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Star formation history of irregular galaxies</style></title><short-title><style face="normal" font="default" size="100%">The Seventh Astrophysical Conference: Star formation, near and far</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">98.56.Si</style></keyword><keyword><style  face="normal" font="default" size="100%">98.56.Wm</style></keyword><keyword><style  face="normal" font="default" size="100%">98.62.Ai</style></keyword><keyword><style  face="normal" font="default" size="100%">98.62.Lv</style></keyword><keyword><style  face="normal" font="default" size="100%">98.62.Qz</style></keyword><keyword><style  face="normal" font="default" size="100%">Dwarf galaxies</style></keyword><keyword><style  face="normal" font="default" size="100%">luminosities</style></keyword><keyword><style  face="normal" font="default" size="100%">Magellanic Clouds and other irregular galaxies</style></keyword><keyword><style  face="normal" font="default" size="100%">Magnitudes and colors</style></keyword><keyword><style  face="normal" font="default" size="100%">morphology and overall structure</style></keyword><keyword><style  face="normal" font="default" size="100%">Origin formation evolution age and star formation</style></keyword><keyword><style  face="normal" font="default" size="100%">radii</style></keyword><keyword><style  face="normal" font="default" size="100%">Stellar content and populations</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1997</style></year><pub-dates><date><style  face="normal" font="default" size="100%">1997/02/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1997AIPC..393..561H</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">393</style></volume><pages><style face="normal" font="default" size="100%">561 - 570</style></pages><isbn><style face="normal" font="default" size="100%">0094-243X</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">Irregular galaxies are generally less massive and less evolved systems than spirals. They constitute a different sort of system in which to study the processes of star formation and galactic evolution. The star formation history of Irregular Galaxies may be affected by several different factors. However, detailed knowledge of the star-formation history of a significant number of objects is necessary before it becomes possible to determine which parameters are important. In the last few years, there has been significant progress on this front. For the first time, we begin to probe in some detail the star-formation history of a fair number of resolved Irregulars in the Local Group. In the present, these results are summarized.</style></abstract></record></records></xml>