Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-26T05:30:57.724Z Has data issue: false hasContentIssue false
  • English
  • Français

Understanding AGB Carbon Star Nucleosynthesis from Observations

Published online by Cambridge University Press:  05 March 2013

C. Abia ,
I. Domínguez ,
R. Gallino ,
M. Busso ,
O. Straniero ,
P. de Laverny  and
G. Wallerstein
C. Abia
Affiliation:
Dpto. Física Teórica y del Cosmos, Universidad de Granada, 18071 Granada, Spain; cabia@ugr.es
I. Domínguez
Affiliation:
Dpto. Física Teórica y del Cosmos, Universidad de Granada, 18071 Granada, Spain; inma@ugr.es
R. Gallino
Affiliation:
Dpto. di Fisica Generale, Universitá di Torino, 10125 Torino, Italy. gallino@ph.unito.it
M. Busso
Affiliation:
Dpto. di Fisica, Universitá di Perugia, 06123 Perugia, Italy. busso@fisica.unipg.it
O. Straniero
Affiliation:
Osservatorio di Collurania, 64100 Teramo, Italy. straniero@astrte.te.astro.it
P. de Laverny
Affiliation:
Observatoire de la Côte d'Azur, UMR6528, 06304 Nice Cedex 4, France. laverny@obs-nice.fr
G. Wallerstein
Affiliation:
Dept. of Astronomy, University of Washington, Seattle WA 98195, USA. wall@orca.astro.washington.edu
Rights & Permissions [Opens in a new window]

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.

Recent advances in the knowledge of the evolutionary status of asymptotic giant branch (AGB) stars and of the nucleosynthesis processes occurring in them are discussed, and used to interpret abundance determinations for s-process elements, lithium and CNO isotopes in several types of AGB stars. We focus our attention mainly on carbon-rich AGB stars. By combining these different constraints we conclude that most carbon stars in the solar neighborhood are of low mass (M≤3 M⊙), their abundances being a consequence of the operation of thermal pulses and the third dredge-up. However, the observed abundances in carbon stars of the R and J types cannot be explained by this standard scenario. These stars may not be on the AGB, but possibly in the core-He burning phases; their envelopes may have been polluted with nuclear ashes of the core-He flash, followed by CNO re-processing enhancing 13C. Observational evidence suggesting the operation of non-standard mixing mechanisms during the AGB phase is also discussed.

Keywords

nuclear reactions, nucleosynthesis, abundancesstars: abundancesstars: AGBstars: carbonstars: evolution
Type
Sixth Torino Workshop
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 4 , 2003 , pp. 314 - 323
Copyright
Copyright © Astronomical Society of Australia 2003

References

Abia, C. et al. 2003, in preparationGoogle Scholar
Abia, C., Domínguez, I., Gallino, R., Busso, M., Masera, S., Straniero, O., de Laverny, P., Plez, B., & Isern, J. 2002, ApJ, 579, 817 Google Scholar
Abia, C., Busso, M., Gallino, R., Domínguez, I., Straniero, O., & Isern, J. 2001, ApJ, 559, 1117 CrossRefGoogle Scholar
Abia, C., & Isern, J. 2000, ApJ, 536, 438 Google Scholar
Abia, C., & Isern, J. 1997, MNRAS, 289, L11 Google Scholar
Abia, C., Boffin, H. M. J., Rebolo, R., & Isern, J. 1993, A&A, 272, 455 Google Scholar
Abia, C., & Wallerstein, G. 1989, MNRAS, 293, 89 CrossRefGoogle Scholar
Amari, S., Nittler, L. R., Zinner, E., & Lewis, R. S. 1997, Lunar Planet. Sci., 28, 33 Google Scholar
Aoki, W., & Tsuji, T. 1997, A&A, 317, 845 Google Scholar
Barbaum, C., Morris, M., & Kahane, C. 1995, ApJ, 450, 862 Google Scholar
Beer, H., & Macklin, R. L. 1989, ApJ, 339, 962 Google Scholar
Bergeat, J., Knapik, A., & Rutily, B. 2002, A&A, 390, 967 Google Scholar
Boothroyd, A. I., & Sackmann, I. 1999, ApJ, 510, 232 Google Scholar
Busso, M., Nollet, K. M., & Wasserburg, G. J. 2002, in Proceedings of the 11th Workshop on Nuclear Astrophysics, eds. Hillebrandt, W., & Müller, E. Max-Planck-Institut für Astrophysik p. 18 Google Scholar
Busso, M., Lambert, D. L., Gallino, R., Travaglio, C., & Smith, V. V. 2001, ApJ, 557, 802 Google Scholar
Busso, M., Gallino, R., & Wasserburg, G. J. 1999, ARA&A, 37, 239 Google Scholar
Cameron, A. G. W., & Fowler, W. A. 1971, ApJ, 161, 111 CrossRefGoogle Scholar
Charbonnel, C. 1995, ApJ, 453, L41 Google Scholar
Charboneel, C., & Balachandran, S. 2000, A&A, 359, 563 Google Scholar
Claussen, M. J., Kleinmann, S. G., Joyce, R. R., & Jura, M. 1987, ApJS, 65, 385 CrossRefGoogle Scholar
Cole, P. W., & Deupree, R. G. 1980, ApJ, 239, 284 Google Scholar
de Laverny, P., & Gustafsson, B. 1999, A&A, 346, 520 Google Scholar
de Laverny, P., & Gustafsson, B. 1998, A&A, 332, 661 Google Scholar
Dominy, J. 1984, PASP, 97, 1104 Google Scholar
Frost, C. A., Cannon, R. C., Lattanzio, J. C., Wood, P. R., & Forestini, M. 1998, A&A, 332, L17 Google Scholar
Gallino, R., Arlandini, C., Busso, M., Lugaro, M., Travaglio, C., Straniero, O., Chieffi, A., & Limongi, M. 1998, ApJ, 497, 388 CrossRefGoogle Scholar
Gilroy, K., & Brown, J. A. 1991, ApJ, 371, 578 Google Scholar
Gratton, R., Sneden, C., Carretta, E., & Bragaglia, A. 2000, A&A, 354, 169 Google Scholar
Gustafsson, B., & Ryde, N. 1996, in IAU Symposium No. 177. ed. Wing, R., p. 481 Google Scholar
Harris, M. J., Lambert, D. L., Hinkle, K. H., Gustafsson, B., & Eriksson, K. 1987, ApJ, 316, 294 Google Scholar
Hatzidimitriou, D., Morgan, D. H., Cannon, R. D., & Croke, B. F. W. 2003, MNRAS, in pressGoogle Scholar
Hauschildt, P. H., Allard, F., Ferguson, J., Baron, E., & Alexander, D. R. 1999, ApJ, 525, 871 Google Scholar
Iben, I. Jr., & Renzini, A. 1983, ARA&A, 21, 271 Google Scholar
Johnson, H. R. 1982, ApJ, 260, 254 Google Scholar
Jorissen, A., Frayer, D. T., Johnson, H. R., Mayor, M., & Smith, V. V. 1993, A&A, 271, 463 Google Scholar
Keenan, P. C. 1993, PASP, 105, 905 Google Scholar
Keenan, P. C., & Boeshaar, P. C. 1980, ApJS, 43, 379 Google Scholar
Kipper, T., Jörgensen, U. G., Klochkova, V. G., & Panchuk, V. E. 1996, A&A, 306, 489 Google Scholar
Kipper, T., & Jörgensen, U. G. 1994, A&A, 290, 148 Google Scholar
Knapp, G. R., Pourbaix, D., & Jorissen, A. 2001, A&A, 371, 222 Google Scholar
Lambert, D. L., Gustafsson, B., Eriksson, K., & Hinkle, K. H. 1986, ApJS, 62, 373 CrossRefGoogle Scholar
Le Bertre, T. 1997, A&A, 176, 107 Google Scholar
Little, S. J., Little-Marenin, I. R., & Hagen, W. 1987, AJ, 94, 981 CrossRefGoogle Scholar
Lorenz-Martins, S. 1996, A&A, 314, 209 Google Scholar
Luck, R. E., & Bond, H. E. 1991, ApJS, 77, 515 CrossRefGoogle Scholar
McClure, R. D. 1997, PASP, 109, 256 Google Scholar
McClure, R. D., & Woodsworth, A.W. 1990, ApJ, 352, 709 Google Scholar
Mengel, J. G., & Gross, P.G. 1976, Astroph., & Space Sci., 41, 70 Google Scholar
Nittler, L. R. et al. 1995, ApJ, 453, L25 Google Scholar
Nollett, K. M., Busso, M., & Wasserburg, G. 2003, ApJ, 582, 1036 Google Scholar
Ohnaka, K., & Tsuji, T. 1998, A&A, 335, 1018 Google Scholar
Ohnaka, K., & Tsuji, T. 1996, A&A, 310, 933 Google Scholar
Parthasarathy, M. 1999, in IAU Symposium No. 191, eds. T. Le Bertre, A. Lébre and C. Waelkens, p. 475 Google Scholar
Pavlenko, Y. 2003, Astron. Reports, 59, 67 Google Scholar
Plez, B. 1999, in Asymptotic Giant Branch Stars, IAU Symp. 191, eds. T. Le Bertre, A. Lèbre, & C. Waelkens, (San Francisco: ASP), 75 Google Scholar
Pourbaix, D., Knapp, G. R., Platais, I., & Jorissen, A. 2003, A&A, (in press)Google Scholar
Sackmann, I. J., & Boothroyd, A. I. 1992, ApJ, 393, L21 Google Scholar
Schöier, F. L., & Olofsson, H. 2000, A&A, 359, 586 Google Scholar
Schwarzschild, M., & Härm, R. 1965, ApJ, 145, 496 Google Scholar
Smith, V. V., & Lambert, D. L. 1990, ApJS, 72, 387 Google Scholar
Straniero, O., Gallino, R., Busso, M., Chieffi, A., Raiteri, C. M., Salaris, M., & Limongi, M. 1995, ApJ, 440, L85 Google Scholar
Utsumi, K. 1985, in Cool Stars with Excesses of Heavy Elements, eds. M. Jascheck & P. C. Keenan (Dordrecht: Reidel), p. 243 Google Scholar
Utsumi, K. 1970, PASJ, 22, 93 Google Scholar
Vandervort, G. L. 1958, AJ, 63, 477 Google Scholar
van Loon, J. Th. et al. 1998, A&A, 329, 169 Google Scholar
van Winckel, H., & Reyniers, C. 2000, A&A, 354, 135 Google Scholar
Vanture, A. D. 1992a, AJ, 103, 2035 CrossRefGoogle Scholar
Vanture, A. D. 1992b, AJ, 104, 1997 Google Scholar
Vanture, A. D. 1992c, AJ, 104, 1986 Google Scholar
Wallerstein, G. 1989, ApJS, 91, 341 Google Scholar
Wallerstein, G., & Knapp, G. R. 1998, ARA&A, 36, 369 Google Scholar
Wasserburg, G. J., Boothroyd, A. I., & Sackmann, I.-J. 1995, ApJ, 440, L101 Google Scholar
Weiss, A., Denissenkov, P. A., & Charbonnel, C. 2000, A&A, 356, 181 Google Scholar
Zinner, E. 1998, ARE&PS, 26, 147 Google Scholar