Hostname: page-component-8448b6f56d-sxzjt Total loading time: 0 Render date: 2024-04-20T01:10:13.771Z Has data issue: false hasContentIssue false
  • English
  • Français

Philosophy of classification for WN stars

Published online by Cambridge University Press:  07 August 2017

Lindsey F. Smith ,
Michael M. Shara  and
Anthony F.J. Moffat
Lindsey F. Smith
Affiliation:
1 School of Physics, University of Sydney, Australia
Michael M. Shara
Affiliation:
2 Space Telescope Science Institute, Baltimore, MD, U.S.A.
Anthony F.J. Moffat
Affiliation:
3 Department de Physique, Université de Montreal, Canada

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The unsatisfactory present state of the classification system for WN stars is summarised and the three dimensions of a new system are presented and justified.

Keywords

stars: Wolf-Rayetclassification
Type
Session I - Basic parameters, properties of single Wolf-Ray et stars
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 48 - 49
Copyright
Copyright © Kluwer 1995 

References

Beals, C.S. 1938, Trans. IAU 6, 248 Google Scholar
Crowther, P.A., Hillier, D.J., Smith, L.J. 1994, A&A in press Google Scholar
Conti, P.S., Leep, E.M., Perry, D.N. 1983, ApJ 268, 228 Google Scholar
Hamann, W.-R., Koesterke, L., Wessolowski, U. 1993, A&A 274, 397 Google Scholar
Hiltner, W.A., Schild, R.E. 1966, ApJ 143, 770 Google Scholar
Smith, L.F. 1968, MNRAS 138, 109 Google Scholar
Smith, L.F. 1973, in: Bappu, M.H.V. & Sahade, J. (eds.), Wolf-Rayet and High Temperature Stars, Proc. IAU Symp. No. 49 (Dordrecht: Reidel), p. 15 Google Scholar
Smith, L.F., Shara, M.M., Moffat, A.F.J. 1990, ApJ 348, 471 Google Scholar