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S Doradus Type; Hubble-Sandage Variables

Published online by Cambridge University Press:  04 August 2017

B. Wolf
B. Wolf*
Affiliation:
Landessternwarte, Königstuhl, 6900 Heidelberg, West Germany

Abstract

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The luminous S Dor variables or Hubble-Sandage variables have gained considerable interest during the past few years for their exceptional (if compared to normal luminous hot stars) stellar wind properties. They seem to represent a short intermezzo in the evolution of the very massive stars prior to becoming WR stars. More recent results on S Dor variables (mainly of the LMC) are briefly summarized. Since most of the data have been or are going to be published elsewhere only an outline will be presented here.

Type
Session 3. Luminous Blue Variables
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 151 - 156
Copyright
Copyright © Reidel 1986 

References

Appenzeller, I., Wolf, B.: 1982, in ESO Workshop “The Most Massive Stars”, p. 131, eds. D'Odorico, S., Baade, D., Kjär, K. Google Scholar
Appenzeller, I.: 1986 (this volume) Google Scholar
Hubble, E., Sandage, A.: 1953, Astrophys. J. 118, 353 CrossRefGoogle Scholar
Humphreys, R. M., Davidson, K.: 1979, Astrophys. J. 232, 409 CrossRefGoogle Scholar
Humphreys, R. M., Blaha, C., D'Odorico, S., Gull, T. R., Benvenuti, P.: 1984, Astrophys. J. 278, 124 Google Scholar
Leitherer, C. et al.: 1986 (this volume) Google Scholar
Leitherer, C., Appenzeller, I., Klare, G., Lamers, H.J.G.L.M. Stahl, O., Waters, L.B.F.M., Wolf, B.: 1985, Astron. Astrophys. (in preparation) Google Scholar
Maeder, A.: 1983, Astron. Astrophys. 120, 113 Google Scholar
Sharov, A. S.: 1975, IAU Symposium 67, Variable Stars and Stellar Evolution, eds. Sherwood, V. E. and Plant, L., D. Reidel, Dordrecht, p. 275 Google Scholar
Stahl, O., Wolf, B.: 1982, Astron. Astrophys. 110, 272 Google Scholar
Stahl, O., Wolf, B., Klare, G., Cassatella, A., Krautter, J., Persi, P., Ferrari-Toniolo, M.: 1983, Astron. Astrophys. 127, 49 Google Scholar
Stahl, O., Wolf, B., de Groot, M., Leitherer, C.: 1985, Astron. Astrophys. Suppl. (in press) Google Scholar
Stahl, O., Wolf, B.: 1985, Astron. Astrophys. (in preparation) Google Scholar
Sterken, C., Wolf, B.: 1978, Astron. Astrophys. 70, 641 Google Scholar
Thackeray, A. D.: 1974, Mon. Not. R. Astron. Soc. 168, 221 CrossRefGoogle Scholar
Walborn, N. R.: 1982, Astrophys. J. 256, 452 CrossRefGoogle Scholar
Waters, L. B. F. M.: 1984, Astron. Astrophys. (in press) Google Scholar
Wolf, B., Appenzeller, I., Cassatella, A.: 1980, Astron. Astrophys. 88, 15 Google Scholar
Wolf, B., Stahl, O.: 1983, The Messenger No. 33, pg. 11 CrossRefGoogle Scholar
Wolf, B., Appenzeller, I., Stahl, O.: 1981, Astron. Astrophys. 103, 94 Google Scholar