Hostname: page-component-77c89778f8-7drxs Total loading time: 0 Render date: 2024-07-18T11:23:11.168Z Has data issue: false hasContentIssue false
  • English
  • Français

Summary and Future Directions

Published online by Cambridge University Press:  12 April 2016

J. M. Marlborough
J. M. Marlborough*
Affiliation:
Department of Physics and Astronomy, The University of Western Ontario, London, Ontario, Canada, N6A 3K7

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.

A summary of the Alicante meeting, entitled The Be Phenomenon in Early Type Stars, is presented here. The emphasis at this meeting was on Be stars, but possible connections to other types of stars were also considered. Some suggestions for the directions of future approaches are provided. The meeting was dedicated to the late Mercedes Jaschek, Carlos Jaschek, and Arne Slettebak, all of whom made significant contributions to our current understanding of Be stars.

Type
8. Summary
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 743 - 751
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Abt, H.A., Tan, H., and Zhou, H. 1997, ApJ, 487, 365 Google Scholar
Clayton, G.C., and Marlborough, J.M. 1980, ApJ, 242, 165 Google Scholar
Dominy, J.F., and Smith, M.A. 1977, ApJ, 217, 494 Google Scholar
Gulliver, A.F. 1981, ApJ, 248, 222 Google Scholar
Gummersbach, C.A., Zickgraf, F.-J., and Wolf, B. 1995, A&A, 302, 409 Google Scholar
Hanuschuk, R.W. 1987, A&A, 173, 299 Google Scholar
Hanuschik, R.W., Hummel, W., Dietle, O., and Sutorius, E. 1995, A&A, 300, 163 Google Scholar
Hirata, R. 1995, PASJ, 47, 195 Google Scholar
Hony, S., Waters, L.B.F.M., Zaal, P.A., de Koter, A., Marlborough, J.M., Millar, C.E., Trams, N.R., Morris, P.W., and de Graauw, Th. 2000, A&A, 357, 1013 Google Scholar
Hubert, A.M., and Floquet, M. 1998, A&A, 335, 565 Google Scholar
Hummel, W., and Hanuschik, R.W. 1997, A&A, 320, 852 Google Scholar
Iglesias, C.A., and Rogers, F.J. 1991, ApJ, 371, 408 CrossRefGoogle Scholar
Jaschek, M., Jaschek, C., and Egret, D. 1986, A&A, 158, 325 Google Scholar
Kriz, S., and Harmanec, P. 1975, BAIC, 26, 65 Google Scholar
Lamers, H.J.G.L.M., and Pauldrach, A.W.A. 1991, A&A, 244, L5 Google Scholar
Millar, C.E., and Marlborough, J.M. 1999, ApJ, 516, 276 Google Scholar
Okazaki, A.T. 1991, PASJ, 43, 75 Google Scholar
Pamyatnykh, A. 1998, in Variable and Non-spherical Stellar Winds in Luminous Hot Stars, eds. Wolf, B., Stahl, O., and Fullerton, A.W., Springer-Verlag, Berlin, p. 320 Google Scholar
Porter, J.M. 1999, A&A, 348, 512 Google Scholar
Rivinius, Th., Baade, D., Stefl, S., Stahl, O., Wolf, B., and Kaufer, A. 1998, A&A, 333, 125 Google Scholar
Seaton, M.J., Yan, Yu, Mihalas, D., and Pradhan, A.K. 1994, MNRAS, 266, 805 Google Scholar
Slettebak, A. 1987, in Physics of Be Stars, eds. Slettebak, A. and Snow, T.P., Cambridge University Press, Cambridge, p. 24 Google Scholar
Smith, M.A., and Robinson, R.D. 1999, ApJ, 517, 866 Google Scholar
Smith, M.A., Robinson, R.D., and Corbet, R.H.D. 1998a, ApJ, 503, 877 Google Scholar
Smith, M.A., Robinson, R.D., and Hatzes, A.P. 1998b, ApJ, 507, 945 Google Scholar
Waters, L.B.F.M., and Marlborough, J.M. 1994, in Pulsation, Rotation and Mass Loss in Early-Type Stars, eds. Balona, L.A., Henrichs, H.F. and Le Contel, J.M., Kluwer Academic Publishers, Dordrecht, p.399 CrossRefGoogle Scholar