Hostname: page-component-848d4c4894-xfwgj Total loading time: 0 Render date: 2024-07-03T05:39:50.615Z Has data issue: false hasContentIssue false
  • English
  • Français

Nucleosynthesis in Intermediate-Mass Stars

Published online by Cambridge University Press:  25 May 2016

John C. Lattanzio ,
Cheryl A. Frost ,
Robert C. Cannon  and
Peter R. Wood
John C. Lattanzio
Affiliation:
Department of Mathematics, Monash University, Clayton, Australia
Cheryl A. Frost
Affiliation:
Department of Mathematics, Monash University, Clayton, Australia
Robert C. Cannon
Affiliation:
School of Biological Sciences, Southampton University, Southampton, England
Peter R. Wood
Affiliation:
Mount Stromlo and Siding Springs Observatories, Australian National University, Canberra, Australia

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.

We discuss nucleosynthesis within 6 M⊙ models with Z = 0.02, 0.008 and 0.004. The emphasis is on the AGB phase of evolution, with particular reference to thermal pulses and Hot Bottom Burning. We find strong CN cycling, with substantial Al production, especially at low metallicities.

Type
Session X — Nucleosythesis and Evolution
Information
Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 449 - 458
Copyright
Copyright © Kluwer 2000 

References

Boothroyd, A. I. & Sackmann, I.-J. 1992, ApJ, 393, L21 Google Scholar
Cannon, R. C. 1993, MNRAS, 263, 817 Google Scholar
Cannon, R. C., Frost, C. A., Lattanzio, J. C. & Wood, P. R. 1998, in preparation Google Scholar
Frost, C. A. & Lattanzio, J. C. 1996a, ApJ, 473, 383 Google Scholar
Frost, C. A. & Lattanzio, J. C. 1996b, in Stellar Evolution: What Should Be Done?, Proceedings of the 32nd Liège Colloquium, ed. Noels, A. et al., p. 307 Google Scholar
Groenewegen, M. A. T. & de Jong, T. 1993, A&A, 267, 410 Google Scholar
Käppeler, F., Wiescher, M., Giesen, U., Görres, J., Baraffe, I., El Eid, M., Raiteri, C. M., Busso, M., Gallino, R., Limongi, M. & Chieffi, A. 1994, ApJ, 437, 396 CrossRefGoogle Scholar
Lattanzio, J. C., Frost, C. A., Cannon, R. C. & Wood, P. R. 1996, Mem. Astron. Soc. Italia, 67, 729 Google Scholar
Mowlavi, N., Jorissen, A. & Arnould, M. 1996, A&A, 311, 803 Google Scholar
Rogers, F. J. & Iglesias, C. A. 1992, ApJ Supp., 79, 507 Google Scholar
Straniero, O., Gallino, R., Busso, M., Chieffi, A., Raiteri, C. M., Limongi, M. & Salaris, M. 1995, ApJ, 440, L85 Google Scholar
Thielemann, F.-K., Arnould, M. & Truran, J. W. 1987, in Advances in Nuclear Astrophysics, ed. Vangioni-Flam, E. et al. (Editions Frontiers: Gif-sur-Yvette), p. 525 Google Scholar
van Loon, J. Th., Zijlstra, A. A., Whitelock, P. A., Loup, C. & Waters, L.B.F.M. 2000, in IAU Symp. 177: The Carbon Star Phenomenon, ed. Wing, R. F. (Kluwer), p. 145 Google Scholar
Vassiliadis, E. & Wood, P. R., 1993, ApJ, 413, 641 Google Scholar
Zinner, E. K. 1995, in Nuclei in the Cosmos III, ed. Busso, M., Gallino, R. and Raiteri, C.M., (AIP Press: New York), p. 567 Google Scholar