Skip to main content
Log in

Further results on the line-profile variability of WR 134

  • Session 3 Spectroscopic Observations of Structure in Winds of WR-Stars
  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

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.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • McCandliss, S.R.: 1988,On the Analysis of Line Profile Variations: a Statistical Approach, University of Colorado: Ph.D. Thesis

  • 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, 214

  • McCandliss, S.R.: 1993, these proceedings

  • Moffat, A.F., Drissen, L., Lamontagne, R., Robert, C.: 1988,ApJ 334, 1038

    Google Scholar 

  • Underhill, A.B., Gilroy, K.K., Hill, G.M., Dinshaw, N.: 1990,ApJ 351, 666

    Google Scholar 

  • Vreux, J.-M., Gosset, E., Bohannan, B., Conti, P.: 1992,A&A 256, 148

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Gosset, E., Vreux, J.M. & Andrillat, Y. Further results on the line-profile variability of WR 134. Astrophys Space Sci 221, 181–188 (1994). https://doi.org/10.1007/BF01091151

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01091151

Key words

Navigation