<?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%">Vasilopoulos, G.</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%">Maggi, P.</style></author><author><style face="normal" font="default" size="100%">Udalski, A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Swift J045558.9-702001, a new HMXB in the LMC</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%">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%">2013/11/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2013ATel.5540....1V</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">5540</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%">We report a new high-mass X-ray binary (HMXB), found in a Swift observation performed on 2013 October 11 as part of the monitoring of the nova LMC2012 (ObsId: 00049549004). The Swift/XRT count rate was 0.023±0.008 cts s&lt;SUP&gt;-1&lt;/SUP&gt;, corresponding to a flux of 1.6×10&lt;SUP&gt;-12&lt;/SUP&gt; erg cm&lt;SUP&gt;-2&lt;/SUP&gt; s&lt;SUP&gt;-1&lt;/SUP&gt; (0.3-10 keV) and an unabsorbed luminosity of 5.1×10&lt;SUP&gt;35&lt;/SUP&gt; erg s&lt;SUP&gt;-1&lt;/SUP&gt; for LMC distance (50 kpc).</style></abstract></record></records></xml>