No CrossRef data available.
Article contents
The Wolf-Rayet Connection - Luminous Blue Variables and Evolved Supergiants
Published online by Cambridge University Press: 03 August 2017
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.
The physical characteristics and behavior of evolved massive stars in three different mass ranges are reviewed with application to whether they may eventually evolve to the WR stage 1. >40-50 M⊙ as LBV's, 2. ∼30-40 M⊙ as cool hypergiant-OH/IR stars and 3. ∼10-30 M⊙ as red supergiant-OH/IR stars. I emphasize the importance of the relatively short but high mass loss phases as LBV's and as OH/IR stars in determining the fate of massive stars from 10 to 100 M⊙.
- Type
- Session VII. Evolution
- Information
- Copyright
- Copyright © Kluwer 1991
References
Appenzeller, I. (1986), IAU Symposium #116, Luminous Stars and Associations in Galaxies, pg. 139.Google Scholar
Conti, P.S., Garmany, C. D., de Loore, C. and Vanbeveren, D. (1983), Astrophys. J.
274, 302.Google Scholar
Davidson, K., Dufour, R.J., Walborn, N.R. and Gull, T.R. (1986), Astrophys. J.
305, 867.Google Scholar
Davidson, K., Walborn, N.R. and Gull, T.R. (1982), Astrophys. J. (Letters)
254, L47.CrossRefGoogle Scholar
de Jager, C., Nieuwenhuijsen, H. and van der Hucht, K. (1988), Astron. Astrophys.
193, 375.Google Scholar
Elias, J.H., Frogel, J.A. and Schwering, P.R.W. (1986), Astrophys. J.
302, 675.CrossRefGoogle Scholar
Fransson, C., Cassatella, A.
Gilmozzi, R., Kushner, R.P., Panagia, N., Sonneborn, G. and Wamsteker, W. (1989), Astrophys. J.
336, 429.Google Scholar
Giguere, P.T., Woolf, N.J. and Webber, J.C. (1976), Astrophys. J. (Letters)
207, L195.Google Scholar
Humphreys, R.M., Blaha, C., D'Odorico, S., Gull, T.R. and Benvenuti, P. (1984), Astrophys. J.
278, 124.Google Scholar
Humphreys, R.M. and Davidson, K., Stahl, O., Wolf, B. and Zickgraf, F.-J. (1989), IAU Colloquium #113, Physics of Luminous Blue Variables, p. 303.Google Scholar
Humphreys, R.M., Strecker, D.W., Murdock, T.L. and Low, F.J. (1973), Astrophys. J. (Letters)
179, L49.CrossRefGoogle Scholar
Humphreys, R.M., Strecker, D.W. and Ney, E.P. (1971), Astrophys. J. (Letters)
167, L35.Google Scholar
Lamers, H.J.G.L.M. (1986), IAU Symposium #116, Luminous Stars and Associations in Galaxies, p. 157.Google Scholar
Lamers, H.J.G.L.M. (1987), in Workshop on Instabilities in Luminous Early-Type Stars, p. 99.Google Scholar
Lamers, H.J.G.L.M. (1989), IAU Colloquium #113, Physics of Luminous Blue Variables, p. 135.Google Scholar
Leitherer, C., Appenzeller, I., Klare, G., Lamers, H.J.G.L.M., Stahl, O., Waters, L.B.F.M. and Wolf, B. (1985), Astron. Astrophys.
120, 113.Google Scholar
Lewis, B.M., Terzian, Y. and Eder, J. (1986), Astrophys. J. (Letters)
302, L23.CrossRefGoogle Scholar
Moffat, A.F.J. (1989), IAU Colloquium #113, Physics of Luminous Blue Variables, p. 229.Google Scholar
Smith, L.J., Pettine, M., Dyson, J.E. and Hartquist, T.W. (1988), Mon. Not. Roy. Astron. Soc.
234, 625.CrossRefGoogle Scholar
Stahl, O., Wolf, B., Leitherer, C., Zickgraf, F.-J., Krautter, J. and de Groot, M. (1984), Astron. Astrophys.
140, 459.Google Scholar
Stahl, O., Wolf, B., Klare, G., Juttner, A. and Cassatella, A., Astron. Astrophys., 228, 379.Google Scholar
van der Hucht, K.A., Hidayat, B., Admiranto, A.G., Supelli, K.R. and Doom, C. (1988), Astron. Astrophys.
199, 217.Google Scholar
Walborn, N.R. (1988), IAU Colloquium #108, Atmospheric Diagnostics of Stellar Evolution, p. 70.Google Scholar
Wood, P.R., Bessell, M.S. and Whiteoak, J.B. (1986), Astrophys. J. (Letters)
306, L81.CrossRefGoogle Scholar
You have
Access