Hostname: page-component-76fb5796d-x4r87 Total loading time: 0 Render date: 2024-04-28T06:06:25.228Z Has data issue: false hasContentIssue false
  • English
  • Français

Circulation and Mixing

Published online by Cambridge University Press:  14 August 2015

R. Kippenhahn
R. Kippenhahn*
Affiliation:
Universitäts-Sternwarte, Göttingen, F.R.G.

Extract

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.

In the preceding lecture Dr Arnett has shown us how exciting the inner life of a star can be when during late stages of evolution higher nuclear reactions take place. But in order to enjoy the variety of different nuclear species formed there stellar material from the deep interior has to be brought up to the surface, where the observers can see it.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 66: Late Stages of Stellar Evolution , 1974 , pp. 20 - 40
Copyright
Copyright © Reidel 1974 

References

Aller, L. H.: 1961, The Abundance of the Elements, Interscience Publ. Inc., New York.Google Scholar
Baker, N. and Kippenhahn, R.: 1959, Z. Astrophys. 48, 140.Google Scholar
Biermann, P.: 1968, Diplomarbeit.Google Scholar
Demarque, P. and McClure, R. D.: 1973, Monthly Notices Roy. Astron. Soc. 164, 5.CrossRefGoogle Scholar
Eddington, A. S.: 1925, Observatory 48, 73.Google Scholar
Finzi, A. and Wolf, R. A.: 1968, Astrophys. J. 153, 865.CrossRefGoogle Scholar
Fricke, K. J.: 1968, Z. Astrophys. 68, 317.Google Scholar
Fricke, K. J. and Kippenhahn, R.: 1972, Ann. Rev. Astron. Astrophys. 10, 45.CrossRefGoogle Scholar
Goldreich, P. and Schubert, G.: 1967, Astrophys. J. 150, 571.CrossRefGoogle Scholar
Gurm, H. S. and Wentzel, D. G.: 1967, Astrophys. J. 149, 139.CrossRefGoogle Scholar
Kippenhahn, R.: 1963, in Gratton, L. (ed.), Star Evolution, Acad. Press. New York, p. 330.Google Scholar
Kippenhahn, R.: 1967, Z. Astrophys. 67, 271.Google Scholar
Kippenhahn, R.: 1969, Astron. Astrophys, 2, 309.Google Scholar
Kippenhahn, R. and Möllenhoff, C.: 1974, Astrophys. Space Sci., in press.Google Scholar
Köhler, H.: 1973, Astron. Astrophys. 25, 467.Google Scholar
Krause, F. and Rädler, K. H.: 1971, in Ergebnisse der Plasmaphysik und der Gaselektronik, Band II, Rompe, R. and Steenbeck, M., Berlin, p. 3.Google Scholar
Mestel, L.: 1953, Monthly Notices Roy. Astron. Soc. 113, 716.Google Scholar
Mestel, L.: 1957, Astrophys. J. 126, 550.Google Scholar
Paczyński, B.: 1973, preprint.Google Scholar
Parker, E. N.: 1970, Ann. Rev. Astron. Astrophys. 8, 1.CrossRefGoogle Scholar
Richstone, D. O.: 1973, preprint.Google Scholar
Rosenbluth, M. N. and Bahcall, J. N.: 1973, Astrophys. J. 184, 9.CrossRefGoogle Scholar
Sackmann, I.-J. and Weidemann, V.: 1972, Astrophys. J. 178, 427.CrossRefGoogle Scholar
Scalo, J. M. and Ulrich, R. K.: 1973, Astrophys. J. 183, 151.CrossRefGoogle Scholar
Sweet, P. A., 1950, Monthly Notices Roy. Astron. Soc. 110, 548.Google Scholar
Thomas, H.-C.: 1967, Z. Astrophys. 67, 420.Google Scholar
Vogt, H.: 1925, Astron. Nachr. 223, 229.Google Scholar
Weigert, A.: 1966, Z. Astrophys. 64, 395.Google Scholar