<?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%">Maggi, P.</style></author><author><style face="normal" font="default" size="100%">Sturm, R.</style></author><author><style face="normal" font="default" size="100%">Haberl, F.</style></author><author><style face="normal" font="default" size="100%">Vasilopoulos, G.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Confirmation of XMMU J010429.4-723136 as a high-mass X-ray binary</style></title><short-title><style face="normal" font="default" size="100%">The Astronomer's Telegram</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Binary</style></keyword><keyword><style  face="normal" font="default" size="100%">Neutron Star</style></keyword><keyword><style  face="normal" font="default" size="100%">Transient</style></keyword><keyword><style  face="normal" font="default" size="100%">X-Ray</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2013</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2013/12/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2013ATel.5674....1M</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">5674</style></volume><pages><style face="normal" font="default" size="100%">1</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">A series of observations performed with Swift/XRT (Target ID 33042) in the SMC detected a relatively bright X-ray source at the edge of the field of view. The source is consistent with &lt;A href=&quot;http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-ref=VIZ52b176e60783&amp;-out.add=.&amp;-source=J/A%2bA/558/A3/smc_src&amp;recno=3027&quot;&gt;XMMU J010429.4-723136&lt;/A&gt;. It is classified as a high-mass X-ray binary (HMXB) candidate in the XMM-Newton point-source catalogue of the SMC (Sturm et al.</style></abstract></record></records></xml>