Abstract
Peter Conti has a tradition of always talking about 0-type stars at Wolf-Rayet symposia, and Wolf-Rayet stars at 0 star symposia. Since there is no well-developed theory for the origin of the winds of WR stars, it is my pleasure to join Peter’s tradition, and to talk mainly about the theory of radiation driven winds in OB stars. The advantage of OB stars is that there exists a fairly complete wind theory, which agrees well with the available observations. The question is, can the mass loss observed from Wolf-Rayet stars be explained by a version of this wind theory which is scaled to the conditions found in the envelopes of Wolf-Rayet stars? The topics I consider are:
-
The calculated radiation pressure in OB stars, and its dependence on temperature, density, and chemical composition.
-
A comparison between predicted and observed mass loss rates and terminal velocities for OB stars.
-
The applicability of the standard radiation driven wind models to Wolf-Rayet stars.
-
Speculations on how Wolf-Rayet stars achieve their enormous mass loss rates within the context of the radiation pressure mechanism.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Abbott, D.C. 1981. Submitted to Ap. J.
Abbott, D.C., Bieging, J.H., Churchwell, E. 1981. Ap. J., in press.
Cameron, A.G. 1973. In Explosive Nucleosynthesis, ed. D. Arnett and D. Schramm ( Univ. of Texas Press: Austin).
Castor, J.I. 1979. In Mass Loss and Evolution of 0-Type Stars, ed. P.S. Conti and C.W.H. de Loore ( Dordrecht: Reidel).
Castor, J.I., Nussbaumer, H. 1972. MNRAS, 155, p. 293.
Castor, J.I., Abbott, D.C., Klein, R.I. 1975. Ap. J., 195, p. 157.
Hartmann, L., Cassinelli, J.P. 1977. Ap. J., 215, p. 155.
Lucy, L. 1981. Preprint.
Massey, P. 1981. Ap. J., 246, p. 153.
Mihalas, D. 1978. Stellar Atmospheres (W. H. Freeman: San Francisco).
Panagia, N., Macchetto, F. 1982. Astr. Ap., in press.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1982 IAU
About this chapter
Cite this chapter
Abbott, D.C. (1982). The Theory of Radiation Driven Stellar Winds and the Wolf-Rayet Phenomenon. In: De Loore, C.W.H., Willis, A.J. (eds) Wolf-Rayet Stars: Observations, Physics, Evolution. International Astronomical Union/Union Astronomique Internationale, vol 99. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7910-9_24
Download citation
DOI: https://doi.org/10.1007/978-94-009-7910-9_24
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-1470-1
Online ISBN: 978-94-009-7910-9
eBook Packages: Springer Book Archive