<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">M. C. Martins</style></author><author><style face="normal" font="default" size="100%">J P Santos</style></author><author><style face="normal" font="default" size="100%">A. M. Costa</style></author><author><style face="normal" font="default" size="100%">F. Parente</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Transition wavelengths and probabilities for spectral lines of Zr III</style></title><secondary-title><style face="normal" font="default" size="100%">The European Physical Journal D</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2006</style></year></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://www.edpsciences.org/articles/epjd/abs/first/d05530/d05530.html</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">39</style></volume><pages><style face="normal" font="default" size="100%">167-172</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">Wavelengths and oscillator strengths for all dipole-allowed fine-structure transitions in Zr III have been calculated within the Multi-Configuration Dirac-Fock method with QED corrections. These transitions are included in the spectrum of some chemically peculiar stars, like the B-type star Lupi observed by the Hubble space telescope. The results are compared to existing experimental and semi-empirical data.</style></abstract><notes><style face="normal" font="default" size="100%">DOI: 10.1140/epjd/e2006-00101-8 PACS 31.25.Jf - Electron correlation calculations for atoms and ions: excited states. 32.30.Jc - Visible and ultraviolet spectra. 32.70.Cs - Oscillator strengths, lifetimes, transition moments.</style></notes></record></records></xml>