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Evolution of Massive Stars Through Late Evolutionary Phases

Published online by Cambridge University Press:  14 August 2015

Susan A. Lamb
Susan A. Lamb*
Affiliation:
University of California, Los Angeles

Extract

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The theoretical study of the evolution of massive stars has considerable relevance to many branches of observational astronomy. As an example, one may mention, first, the direct application of theoretical models in interpreting the observed properties of supergiants, and second, the use of calculations of the nucleosynthesis taking place in these stars, together with observed supergiant mass loss rates and supernova calculations, to estimate the rate and type of nucleosynthetic enrichment of the interstellar medium by supergiants.

Type
Part VII: Theoretical Papers and Summary
Information
Symposium - International Astronomical Union , Volume 80: The HR Diagram , 1978 , pp. 349 - 356
Copyright
Copyright © Reidel 1978 

References

Arnett, W.D. (1972). Astrophys. J. 176, 699.Google Scholar
Arnett, W.D. (1977). Astrophys. J. Suppl. 35, 127.Google Scholar
Arnett, W.D. (1978). Astrophys. J. (in press).Google Scholar
Beaudet, G., Petrosian, V. and Salpeter, E.E. (1967). Astrophys. J. 150, 979.Google Scholar
Chevalier, R.A. and Kirschner, R.P. (1978). Astrophys. J. (in press).Google Scholar
Chiosi, C., Nasi, E. and Sreenivasan, S.R. (1977). Astron. Astrophys. (in press).Google Scholar
Chiosi, C. and Summa, C. (1970). Astrophys. Space Sci. 8, 478.Google Scholar
Couch, R.G., Schmeidekamp, A.B. and Arnett, W.D. (1974). Astrophys. J. 190, 95.Google Scholar
Endal, A. S. (1975). Astrophys. J. 197, 405.Google Scholar
Ferrari, A., Galeotti, P., Silvestro, G. and Trussoni, E. (1970). Astrophys. Space Sci. 9, 181.Google Scholar
Festa, G.G. and Ruderman, M.A. (1969). Phys. Rev. 180, 1227.Google Scholar
Gascoigne, S.C.B. (1969). Mon. Not. Roy. Astron. Soc. 146, 1.Google Scholar
Hartwick, F.D.A. (1967). Astrophys. J. 150, 953.Google Scholar
Hayashi, C. and Cameron, R.C. (1962). Astrophys. J. 136, 166.Google Scholar
Humphreys, R.M. (1970). Astrophys. Letters 6, 1.Google Scholar
Ikeuchi, S., Nakazawa, K., Murai, T., Hoshi, R. and Hayashi, C. (1971). Prog. Theor. Phys. Kyoto 46, 1713.Google Scholar
Ikeuchi, S., Nakazawa, K., Murai, T., Hoshi, R. and Hayashi, C. (1972). ibid. 48, 1870.Google Scholar
Lamb, S.A. (1978). Astrophys. J. (in press).Google Scholar
Lamb, S.A., Howard, W.M., Truran, J.W. and Iben, I. (1977). Astrophys. J. 217, 213.Google Scholar
Lamb, S.A., Iben, I. and Howard, W.M. (1976). Astrophys. J. 207, 209.Google Scholar
de Loore, C., De Grève, J.P. and Lamers, H.J.G.L.M. (1977). (preprint).Google Scholar
Peimbert, M. (1971). Astrophys. J. 170, 261.Google Scholar
Peimbert, M. and van den Bergh, S. (1971). Astrophys. J. 167, 223.Google Scholar
Rakavy, G., Shaviv, G. and Zinamon, Z. (1967). Astrophys. J. 150, 131.Google Scholar
Stothers, R. (1969). Astrophys. J. 155, 935.CrossRefGoogle Scholar
Stothers, R. and Chin, C.-W. (1969). Astrophys. J. 158, 1039.Google Scholar
Sugimoto, D. (1970). Prog. Theor. Phys. Kyoto 44, 599.Google Scholar
Sugimoto, D. and Nomoto, K. (1974). In IAU Symposium 66, Late Stages of Stellar Evolution, Tayler, R.J. and Hesser, J., eds., Reidel, Dordrecht, p. 105.Google Scholar
Walborn, N. (1976). Astrophys. J. 205, 419.CrossRefGoogle Scholar