Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-23T20:30:11.791Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution and Mixing on the Agb

Published online by Cambridge University Press:  12 April 2016

John C. Lattanzio
John C. Lattanzio*
Affiliation:
Institute of Geophysics and Planetary Physics, Lawrence LivermoreNational Laboratory, L-413, P.O. Box 808, Livermore, Ca., 94550

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.

It is now well known that Nature can make Carbon stars at lower luminosities than can (human) theorists. A number of workers, stimulated by this challenge, have been attracted to the problem. In this paper I review recent evolutionary models of relatively low mass AGB stars, with emphasis placed on the mixing of carbon to the stellar surface. In particular I discuss some recent improvements in the physics used to construct stellar models. These topics include: breathing pulses of the convective core found during core helium exhaustion; the effects of carbon recombination; the occurrence of semiconvection in the region between the two nuclear burning shells; and the importance of mass loss. Recent calculations have successfully produced models of low luminosity Carbon stars. The strengths and weaknesses of these models will be contrasted.

Type
3. Evolution of Peculiar Red Giant Stars
Information
International Astronomical Union Colloquium , Volume 106: Evolution of Peculiar Red Giant Stars , 1989 , pp. 161 - 175
Copyright
Copyright © Cambridge University Press 1989

References

Becker, S.A., and Iben, I. Jr., 1979, Astrophys. J., 232, 831.Google Scholar
Becker, S.A., and Iben, I. Jr., 1980, Astrophys. J., 237, 111.Google Scholar
Bertelli, G., Chiosi, C., and Lattanzio, J.C., 1988, in preparation.Google Scholar
Blanco, B.M., Blanco, V.M., and McCarthy, M.F., 1978, Nature, 271, 638.Google Scholar
Blanco, V.M., McCarthy, M.F., and Blanco, B.M., 1980, Astrophys. J., 242, 948.Google Scholar
Boothroyd, A.I., and Sackmann, I.-J., 1988a, Astrophys. J., 328, 632 (BSl).Google Scholar
Boothroyd, A.I., and Sackmann, I.-J., 1988b, Astrophys. J., 328, 641 (BS2).Google Scholar
Boothroyd, A.I., and Sackmann, I.-J., 1988c, Astrophys. J., 328, 653 (BS3).Google Scholar
Boothroyd, A.I., and Sackmann, I.-J., 1988d, Astrophys. J., 328, 671 (BS4).Google Scholar
Bressan, A., Bertelli, G., Chiosi, C., 1981, Astron. Astrophys., 102, 25.Google Scholar
Castellani, V., Chieffi, A., Pulone, L., and Tornambe, A., 1985a, Astrophys. J. Lett., 296, 204.Google Scholar
Castellani, V., Chieffi, A., Pulone, L., and Tornambe, A., 1985b, Astrophys. J., 294, L31.Google Scholar
Castellani, V., Giannone, P., and Renzini, A., 1971a, Astrophys. Space. Sci, 10, 340.CrossRefGoogle Scholar
Castellani, V., Giannone, P., and Renzini, A., 1971b, Astrophys. Space. Sci, 10, 355.Google Scholar
Chiosi, C., Bertelli, G., and Bressan, A., 1987, in Late Stages of Stellar Evolution, Ed. Kwok, S. & Pottasch, S.R., (Dordrecht: Reidel), 213.CrossRefGoogle Scholar
Cox, A.N., and Stewart, J.N., 1970, Astrophys. J. Suppl. Ser., 19, 261.Google Scholar
Despain, K.H., 1981, Astrophys. J., 251, 639.Google Scholar
Gingold, R.A., 1976, Astrophys. J., 204, 116.Google Scholar
Hollowell, D.E., 1987, in Late Stages of Stellar Evolution, Ed. Kwok, S. & Pottasch, S.R., (Dordrecht: Reidel), 239 (DH1).Google Scholar
Hollowell, D.E., 1988, Ph.D. thesis, University of Illinois (DH2).Google Scholar
Hollowell, D.E., and Iben, I. Jr., 1988, preprint.Google Scholar
Huebner, W.F., Merts, A.L., Magee, N.H. Jr., and Argo, M.F., 1977, Los: Alamos Sdentine Laboratory Report LA-6760-M.Google Scholar
Iben, I. Jr., 1975a, Astrophys. J., 196, 525.Google Scholar
Iben, I. Jr., 1975b, Astrophys. J., 196, 549.Google Scholar
Iben, I. Jr., 1976, Astrophys. J., 208, 165.CrossRefGoogle Scholar
Iben, I. Jr., 1981, Astrophys. J., 246, 278.Google Scholar
Iben, I. Jr., 1982, Astrophys. J., 260, 821.Google Scholar
Iben, I. Jr., 1983, Astrophys. J. Lett, 275, L65.Google Scholar
Iben, I. Jr., 1984, in ObservationaJ Tests of the Stellar Evolution Theory, Ed. Maeder, A. & Renzini, A., (Dordrecht: Reidel), 3.Google Scholar
Iben, I. Jr., 1987, in Late Stages of Stellar Evolution, Ed. Kwok, S. & Pottasch, S.R., (Dordrecht: Reidel), 175.Google Scholar
Iben, I. Jr., and Renzini, A., 1982a, Astrophys. J. Lett, 259, L79 (IR82a).Google Scholar
Iben, I. Jr., and Renzini, A., 1982b, Astrophys. J. Lett., 263, L65 (IR82b).Google Scholar
Iben, I. Jr., and Renzini, A., 1983, Ann. Rev. Astr. Astrophys., 21, 271 (IR83).Google Scholar
Iben, I. Jr., and Renzini, A., 1984, Phys. Rept., 105, 329.Google Scholar
Lattanzio, J.C., 1984, Ph.D. thesis, Monash University, Australia (JL1).Google Scholar
Lattanzio, J.C., 1986, Astrophys. J., 311, 708 (JL2).Google Scholar
Lattanzio, J.C., 1987a, in Late Stages of Stellar Evolution, Ed. Kwok, S. & Pottasch, S.R., (Dordrecht: Reidel), 235 (JL3).Google Scholar
Lattanzio, J.C., 1987b, Astrophys. J. Lett., 313, L15 (JL4).CrossRefGoogle Scholar
Lattanzio, J.C., 1988, in Origin and Distribution of the Elements, Ed. Mathews, G.J., (Singapore: World Scientific), 398Google Scholar
Magee, N.H. Jr., Merts, A.L., and Huebner, W.F., 1975, Astrophys. J., 196, 617.Google Scholar
Mazzitelli, I., and D'Antona, F., 1986, Astrophys. J., 311, 762.Google Scholar
Renzini, A., Bernazanni, M., Buonanno, R., and Corsi, CE., 1985, Astrophys. J. Lett, 294, L7.Google Scholar
Renzini, A., and Fusi Pecci, F., 1988, preprint.Google Scholar
Renzini, A., and Voli, M., 1981, Astron. Astrophys., 94, 175.Google Scholar
Richer, H.B., 1981, Astrophys. J., 243, 744.Google Scholar
Robertson, J.W., and Faulkner, D.J., 1972, Astrophys. J., 171, 309.Google Scholar
Sackmann, I.-J., 1980, Astrophys. J. Lett, 241, L37.Google Scholar
Sackmann, I.-J., and Boothroyd, A.I., 1985, Astrophys. J., 293, 154.Google Scholar
Schonberner, D., 1979, Astron. Astrophys., 79, 108.Google Scholar
Smith, V.V., and Lambert, D.L., 1986, Astrophys. J., 311, 843.Google Scholar
Sweigart, A.V., and Démarque, P., 1972, Astron. Astrophys., 20, 445.Google Scholar
Sweigart, A.V., and Démarque, P., 1973, in Variable Stars in Globular Clusters and Related Systems, Proc. IAU Coll. No. 21, Ed. Fernie, J.D., (Dordrecht: Reidel), 221.Google Scholar
VandenBerg, D.A., 1983, Astrophys. J. Suppl. Ser., 51, 29.Google Scholar
Weidemann, V., and Koester, D., 1983, Astron. Astrophys., 121, 77.Google Scholar
Wood, P.R., 1981, in Physical Processes in Red Giants, Ed. Iben, I. Jr., & Renzini, A., (Dordrecht: Reidel), 135Google Scholar
Wood, P.R., Bessell, M.S., and Fox, M.W., 1983, Astrophys. J., 272, 99.Google Scholar