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Final stages of AGB evolution

Published online by Cambridge University Press:  25 May 2016

P.R. Wood
P.R. Wood*
Affiliation:
Mount Stromlo & Siding Spring Observatories Private Bag, Weston Creek PO, ACT 2611, Australia

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The final stages of AGB evolution still remain difficult to study theoretically. From the stellar point of view, the main theoretical problems are the evolution of the stars (involving shell flashes and dredge-up of carbon and s-process elements), pulsation, and the production of mass loss by pulsation and radiation pressure on grains. In this paper I will discuss these topics. A recent review concentrating more on the circumstellar aspects of AGB evolution is given by Habing (1996).

Type
V. From AGB to Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 297 - 302
Copyright
Copyright © Kluwer 1997 

References

Barnbaum, C., Morris, M. & Kahane, C. 1995, ApJ, 450, 862.Google Scholar
Baud, B., Habing, H., Matthews, H.E. & Winnberg, A. 1981, A&A, 95, 156.Google Scholar
Blöcker, T. 1995, A&A, 297, 727.Google Scholar
Boothroyd, A.I. & Sackmann, I.J. 1988, ApJ, 328, 671.Google Scholar
Bowen, G.H. 1988, ApJ, 329, 299.Google Scholar
Dopita, M.A. et al. 1997, ApJ, in press.Google Scholar
Dorfi, E.A. and Höfner, S. 1996, A&A, 313, 605.Google Scholar
Fleischer, A.J., Gauger, A. & Sedlmayr, E. 1995, A&A, 297, 543.Google Scholar
Frank, A., Balick, B., Icke, V. & Mellema, G. 1993, ApJL, 404, L25.Google Scholar
Frost, C. & Lattanzio, J.C. 1996, ApJ, in press.Google Scholar
Groenewegen, M.A.T. & de Jong, T. 1993, A&A, 267, 410.Google Scholar
Groenewegen, M.A.T. & de Jong, T. 1994a, A&A, 282, 127.Google Scholar
Groenewegen, M.A.T. & de Jong, T. 1994b, A&A, 283, 463.Google Scholar
Habing, H.J. 1996, A&AR, 7, 97.Google Scholar
Habing, H.J., Tignon, J. & Tielens, A.G.G.M. 1994, A&A, 286, 523.Google Scholar
Han, Z., Podsiadlowski, P. & Eggleton, P.P. 1995, MNRAS, 272, 800.Google Scholar
Haniff, C.A., Scholz, M. & Tuthill, P.G. 1995, MNRAS, 276, 400.Google Scholar
Höfner, S., Feuchtinger, M.U. & Dorfi, E.A. 1995, A&A, 297, 815.Google Scholar
Kahane, C., Audinos, P., Barnbaum, C. and Morris, M. 1996, A&A, in press.Google Scholar
Lattanzio, J.C. 1989, ApJ, 347, 989.Google Scholar
Marigo, P., Bressan, A. & Chiosi, C. 1996, A&A, 313, 545.Google Scholar
Netzer, N. & Elitzur, M. 1993, ApJ, 410, 701.Google Scholar
O'Dell, C.R. 1963, Ap.J., 138, 67.Google Scholar
Paczynski, B. 1971, Acta Astr., 21, 417.Google Scholar
Schild, H. 1989, MNRAS, 240, 63.CrossRefGoogle Scholar
Schönberner, D. 1981, A&A, 103, 119.Google Scholar
Soker, N. & Livio, M. 1989, ApJ, 339, 268.Google Scholar
Szczerba, R. & Blommaert, J.A.D.L. 1993, Acta Astr., 43, 397.Google Scholar
Vassiliasis, E. & Wood, P.R. 1993, ApJ, 413, 641.Google Scholar
Weidemann, V. 1987, A&A, 188, 74.Google Scholar
Willson, L.A. 1982, in Pulsations in Classical and Cataclysmic Variable Stars, eds. Cox, J.P. & Hansen, C.J. (Boulder: JILA), p.269.Google Scholar
Winters, J.M., Fleischer, A.J., Gauger, A. & Sedlmayr, E. 1994, A&A, 290, 623.Google Scholar
Wood, P.R. 1981, in Physical Processes in Red Giants, eds. Iben, I. & Renzini, A. (Reidel: Dordrecht), p.135.CrossRefGoogle Scholar
Wood, P.R. 1990, in Confrontation between Stellar Pulsation and Evolution, eds. Cacciari, C. & Clementini, G., ASP Conf. Series, 11, 355.Google Scholar
Wood, P.R. 1996, Mem. Soc. Astron. It., in press.Google Scholar
Wood, P.R. & Sebo, K.M. 1996, MNRAS, 282, 958.Google Scholar
Wood, P.R., Whiteoak, J.B., Hughes, S.M.G., Bessell, M.S., Gardner, F.F. & Hyland, A.R. 1992, ApJ, 397, 552.Google Scholar