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Winds

Published online by Cambridge University Press:  12 April 2016

K.B. MacGregor
K.B. MacGregor*
Affiliation:
High Altitude Observatory/NCAR, *P. O. Box 3000, Boulder, CO 80307, U.S.A.

Abstract

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It is by now well known that most main sequence stars continuously lose mass as a consequence of the winds they emit. In addition to affecting the thermal and dynamical state of the stellar atmosphere, such mass loss can also induce changes in the interiors of stars. In the present review, we consider a few of the ways in which sustained, wind-like mass loss can alter the physical state of main sequence stellar interiors by examining the differences in internal structure, composition, and rotation between mass-losing and conservatively evolving stars.

Type
VII. Activity, a break of spherical symmetry
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 620 - 633
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Abt, H.A., & Levy, S.G. 1985, Ap. J. Suppl., 59, 229 Google Scholar
Aller, L.H. & Chapman, S. 1960, Ap.J., 132, 461 CrossRefGoogle Scholar
Boyarchuk, A.A., & Savanov, I.S. 1986, In Upper Main Sequence Stars with Anomalous Abundances, eds. C.Cowley, , Dworetsky, M.M., and Megessier, C. (Dordrecht: Reidel), p. 433 Google Scholar
Brown, A., Vealé, A., Judge, P., Bookbinder, J.A., & Hubeny, I. 1990, Ap.J., 361, 220 Google Scholar
Brunish, W.M., & Truran, J.W. 1982, Ap.J., 256, 247 Google Scholar
Cassinelli, J.P., & Lamers, H., J.G.⊥, M. 1987, In Exploring the Universe with the IUE Satellite, ed. Kondo, Y. (Dordrecht: Reidel), p. 139 Google Scholar
Castor, J.I., Abbott, D.C., & Klein, R. 1975, Ap. J., 195, 157 Google Scholar
Cayrel, R., Burkhart, C., & Van’t Veer, C. 1991, In Evolution of Stars: The Photospheric Abundance Connection, eds. Michaud, G. and Tutkov, A.(Dordrecht: Reidel), p. 99 CrossRefGoogle Scholar
Chapman, S., & Cowling, T.G. 1970, The Mathematical Theory of Non-Uniform Gases (Cambridge: Cambridge Univ. Press), p. 257 Google Scholar
Charbonneau, P. 1992, In Proceedings of the 7th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, eds. Giampapa, M.S. and Bookbinder, J.A. in pressGoogle Scholar
Charbonneau, P., and MacGregor, K.B. 1992a, Ap. J.,, 387, 639 Google Scholar
Charbonneau, P. -1992b, Ap. J. (Letters), in pressGoogle Scholar
Charbonneau, P. -1992c, these proceedingsGoogle Scholar
Chiosi, C., & Maeder, A. 1986, Ann. Rev. Astr. Ap., 24, 329 CrossRefGoogle Scholar
Chiosi, C., & Nasi, E. 1974, Astr. Ap., 34, 355 Google Scholar
Dearborn, D.S.P., Blake, J.B., Hainebach, K.L., & Schramm, D.N. 1978, Ap. J., 223, 552 Google Scholar
Endal, A.S., & Sofia, S. 1978, Ap. J., 220, 279 CrossRefGoogle Scholar
Endal, A.S., & Sofia, S. 1981, Ap. J., 243, 625 Google Scholar
Falk, H.J. & Mitalas, R. 1981, M.N.R.A.S., 196, 225 Google Scholar
Garmany, C.D., & Conti, P.S. 1984, Ap. J., 284, 705 Google Scholar
Gough, D.O. 1991, In Angular Momentum Evolution of Young Stars, eds. Catalano, S. and Stauffer, J. (Dordrecht: Kluwer), p. 271 CrossRefGoogle Scholar
Hartwick, F.D.A. 1967, Ap. J. 150, 953 Google Scholar
Lanz, T., & Catala, C., 1992, Astr. Ap., 257, 663 Google Scholar
Maeder, A., 1984, In Observational Tests of the Stellar Evolution Theory, eds. Maeder, A. and Renzini, A. (Dordrecht: Reidel), p. 299 CrossRefGoogle Scholar
McCrea, W.H. 1962, Q.J.R.A.S., 3, 63 Google Scholar
Mestel, L., & Weiss, N.O. 1987, M.N.R.A.S., 226,123 Google Scholar
Michaud, G. 1970, Ap. J., 160, 641 Google Scholar
Michaud, G. 1977, In Highlights of Astronomy, Vol. 4, Part II, ed. E.A. Miller, (Dordrecht: Reidel), p. 177 Google Scholar
Michaud, G. 1987, Physica Scripta, 36, 112 Google Scholar
Michaud, G. 1991, In Evolution of Stars: The Photospheric Abundance Connection, eds. Michaud, G. and Tutkov, A. (Dordrecht: Reidel), p.111 Google Scholar
Michaud, G., Charland, Y., Vauclair, S., & Vauclair, G. 1976, Ap. J., 210, 447 Google Scholar
Michaud, G., Tarasick, D., Charland, Y., & Pelletier, C. 1983, Ap. J., 269, 239 CrossRefGoogle Scholar
Mitalas, R., & Falk, H.J. 1984, M.N.R.A.S., 210, 641 Google Scholar
Moss, D.L., Mestel, L., and Tayler, R.J. 1990, M.N.R.A.S., 245, 550 Google Scholar
Pinsonneault, M.H., Kawaler, S.D., Sofia, S., & Demarque, P. 1989, Ap. J., 338, 424 Google Scholar
Pizzo, V., Schwenn, R., Marsch, E., Rosenbauer, H., Mühlhäuse, K.H., Neubauer, F.M., 1983, Ap. J. 271, 335 Google Scholar
Preston, G.W. 1974, Ann. Rev. Astr. Ap., 12, 257 CrossRefGoogle Scholar
Roxburgh, I.W. 1991, In Angular Momentum Evolution of Young Stars, eds. Catalano, S. and Stauffer, J. (Dordrecht: Kluwer), p. 365 Google Scholar
Stauffer, J. 1991, In Angular Momentum Evolution of Young Stars, eds. catalano, S. and Stauffer, J. (Dordrecht: Kluwer) p. 117 Google Scholar
Stein, R.F. 1966, In Stellar Evolution, eds. Stein, R.F. and Cameron, A.G.W. (New York: Plenum), p. 3 Google Scholar
Tanaka, Y. 1966, Pub. Astron. Soc. Japan, 18, 47 Google Scholar
Tassoul, J.-L., & Tassoul, M. 1989, Astr. Ap., 213, 397 Google Scholar
Tassoul, J.-L. 1978, Theory of Rotating Stars (Princeton: Princeton University Press)Google Scholar
Toutain, T., & Fröhlich, C. 1992, Astr. Ap., 257, 287 Google Scholar
Vauclair, S., & Vauclair, G. 1982, Ann. Rev. Astr. Ap., 20, 37 Google Scholar
Watson, W.D. 1970, Ap. J. (Letters), 162, L45 Google Scholar
Watson, W.D. 1971, Astr. Ap., 13, 263 Google Scholar
Weber, E.J., & Davis, L. 1967, Ap. J., 148, 217 Google Scholar
Zahn, J.-P. 1983 in Asrtophysical Processes in Upper Main Sequence Stars(Geneva: Publ. Observatoire Genève), p. 253 Google Scholar