<?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%">Morgan, D. H.</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%">A survey of carbon stars in the Small Magellanic Cloud.</style></title><short-title><style face="normal" font="default" size="100%">Astronomy and Astrophysics Supplement Series</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">MAGELLANIC CLOUD</style></keyword><keyword><style  face="normal" font="default" size="100%">STARS: CARBON SURVEYS</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1995</style></year><pub-dates><date><style  face="normal" font="default" size="100%">1995/11/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1995A&amp;AS..113..539M</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">113</style></volume><pages><style face="normal" font="default" size="100%">539</style></pages><isbn><style face="normal" font="default" size="100%">0365-0138</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">A survey of carbon stars in the outer parts of the Small Magellanic Cloud has been completed; the candidate objects were identified by inspecting UK Schmidt Telescope objective-prism plates which cover a total area of ~220sq.deg on the sky, including the inter-Cloud region. Co-ordinates, accurate to =~2arcsec, are given for 1185 newly identified carbon stars. The spatial distribution of the SMC carbon stars appears to be identical to that of red, horizontal-branch/clump stars found by Gardiner &amp;amp; Hatzidimitriou (1992).</style></abstract></record></records></xml>