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Summary of Symposium

Published online by Cambridge University Press:  03 August 2017

Peter S. Conti
Peter S. Conti*
Affiliation:
Joint Institute for Laboratory Astrophysics University of Colorado, Boulder, CO 80309-0440, USA

Extract

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“It is a significant fact that the emission and absorption lines of Wolf-Rayet spectra cannot be regarded as being formed in one body of gas at one representative temperature and pressure” (Underhill 1968)

“I think it fair to say that the demonstration of… diversity has brought the Wolf-Rayet stars from being a curiosity to being an important part of the ‘main stream’ evolution of all massive stars” (Smith 1982)

Type
Session IX. Summary
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 661 - 668
Copyright
Copyright © Kluwer 1991 

References

REFERENCES

Bappu, M.K.V. and Sahade, J. 1973 Wolf-Rayet and High-Temperature Stars, IAU Symposium #49 (D. Reidel, Dordrecht)CrossRefGoogle Scholar
De Loore, C.W.H. and Willis, A.J. 1982 Wolf-Rayet Stars: Observations, Physics. Evolution, IAU Symposium #99 (D. Reidel, Dordrecht)CrossRefGoogle Scholar
Gebbie, K.B. and Thomas, R.N. 1968 Wolf-Rayet Stars Proceedings of a Symposium, NBS Special Publication 307 (U.S. Government Printing Office, Washington D.C.)CrossRefGoogle Scholar
Smith, L.F. 1982 in Wolf-Rayet Stars: Observations. Physics. Evolution, eds. De Loore, C.W.H. and Willis, A.J. (D. Reidel, Dordrecht), p. 599 Google Scholar
Underhill, A.B. 1968 in Wolf- Rayet Stars, eds. Gebbie, K.B. and Thomas, R.N. (U.S. Government Printing Office, Washington D.C.), p. 185 Google Scholar