Astrophysics and Space Science

, Volume 221, Issue 1–2, pp 181–188 | Cite as

Further results on the line-profile variability of WR 134

  • E. Gosset
  • J. -M. Vreux
  • Y. Andrillat
Session 3 Spectroscopic Observations of Structure in Winds of WR-Stars

Abstract

We discuss a few conclusions previously derived from the analysis of the lineprofile variability of the Wolf-Rayet star WR 134; some details are made more explicit. In addition, we present a new set of data and briefly comment on recent results deduced from its analysis.

Key words

Wolf-Rayet stars: WR 134 Line-profile variability 

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. McCandliss, S.R.: 1988,On the Analysis of Line Profile Variations: a Statistical Approach, University of Colorado: Ph.D. ThesisGoogle Scholar
  2. McCandliss, S.R.: 1992, ‘Line Profile Variations in the Wolf-Rayet Star WR 134’ in L. Drissen, C. Leitherer, A. Nota, ed(s).,Nonisotropic and Variable Outflows from Stars, ASP Conf. Ser. vol. 22: San Francisco, 214Google Scholar
  3. McCandliss, S.R.: 1993, these proceedingsGoogle Scholar
  4. Moffat, A.F., Drissen, L., Lamontagne, R., Robert, C.: 1988,ApJ 334, 1038Google Scholar
  5. Underhill, A.B., Gilroy, K.K., Hill, G.M., Dinshaw, N.: 1990,ApJ 351, 666Google Scholar
  6. Vreux, J.-M., Gosset, E., Bohannan, B., Conti, P.: 1992,A&A 256, 148Google Scholar

Copyright information

© Kluwer Academic Publishers 1994

Authors and Affiliations

  • E. Gosset
    • 1
  • J. -M. Vreux
    • 1
  • Y. Andrillat
    • 2
  1. 1.Institut d'AstrophysiqueUniversité de LiègeBelgium
  2. 2.Laboratoire d'AstronomieUniversité des Sciences Montpellier IIFrance

Personalised recommendations