An extensive spectroscopic time series of three Wolf-Rayet stars - I. The lifetime of large-scale structures in the wind of WR 134

E.~J. Aldoretta, N. St-Louis, N.~D. Richardson, A.~F.~J. Moffat, T. Eversberg, G.~M. Hill, T. Shenar, É. Artigau, B. Gauza, J.~H. Knapen, J. Kubát, B. Kubátová, R. Maltais-Tariant, M. Muñoz, H. Pablo, T. Ramiaramanantsoa, A. Richard-Laferrière, D.~P. Sablowski, S. Simón-Diaz, L. St-JeanF. Bolduan, F.~M. Dias, P. Dubreuil, D. Fuchs, T. Garrel, G. Grutzeck, T. Hunger, D. Küsters, M. Langenbrink, R. Leadbeater, D. Li, A. Lopez, B. Mauclaire, T. Moldenhawer, M. Potter, E.~M. dos Santos, L. Schanne, J. Schmidt, H. Sieske, J. Strachan, E. Stinner, P. Stinner, B. Stober, K. Strandbaek, T. Syder, D. Verilhac, U. Waldschläger, D. Weiss, A. Wendt

Research output: Contribution to journalArticlepeer-review

Original languageUndefined/Unknown
Pages (from-to)3407-3417
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume460
Issue number3
DOIs
StatePublished - Aug 1 2016

Keywords

  • instabilities
  • methods: data analysis
  • techniques: spectroscopic
  • stars: individual: WR 134
  • stars: massive
  • stars: Wolf-Rayet
  • Astrophysics - Solar and Stellar Astrophysics

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