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Hydrogen in the atmosphere of the evolved WN3 Wolf–Rayet star WR 3: defying an evolutionary paradigm?
Authors:S V Marchenko  A F J Moffat  P A Crowther  A-N Chené  M De Serres  P R J Eenens  G M Hill  J Moran  T Morel
Institution:Department of Physics and Astronomy, Western Kentucky University, Bowling Green, KY 42101-3576, USA;Département de Physique, Universitéde Montréal, C.P. 6128, Succ. 'Centre-Ville', Montréal, QC, H3C 3J7, Canada, and Observatoire du mont Mégantic;Department of Physics and Astronomy, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH;Physics Department, McGill University, Rutherford Physics Building, 3600 University St, Montreal, QC, H3A 2T8, Canada;Institut d'Astrophysique, Universitéde Liège, Allée du 6 Août 17 (B5C), B - 4000 Liège (Sart Tilman), Belgium;Department of Astronomy, University of Guanajuato, 36000 Guanajuato, GTO, Mexico;W.M. Keck Observatory, 65-1120 Mamalahoa Hwy, Kamuela, HI 96743, USA;Department of Physics and Astronomy, University of North Carolina, Phillips Hall, CB #3255, Chapel Hill, NC 27599-3255, USA;Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Palermo G.S. Vaiana, Piazza del Parlamento 1, I-90134 Palermo, Italy
Abstract:
Keywords:stars: abundances  stars: individual: WR 3  stars: Wolf–Rayet
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