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Galactic Chemical Evolution of the s Process from AGB Stars

Published online by Cambridge University Press:  05 March 2013

Alessandra Serminato*
Affiliation:
Dipartimento di Fisica Generale, Università di Torino, via P. Giuria, 1, 10125 Torino, Italy
Roberto Gallino
Affiliation:
Dipartimento di Fisica Generale, Università di Torino, via P. Giuria, 1, 10125 Torino, Italy
Claudia Travaglio
Affiliation:
Osservatorio Astronomico di Torino (INAF), Strada Osservatorio 20, 10025 Pino Torinese, Italy
Sara Bisterzo
Affiliation:
Dipartimento di Fisica Generale, Università di Torino, via P. Giuria, 1, 10125 Torino, Italy
Oscar Straniero
Affiliation:
Osservatorio Astronomico di Collurania (INAF), via M. Maggini, Teramo 64100, Italy
*
DCorresponding author. Email: [email protected]
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Abstract

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We follow the chemical evolution of the Galaxy for the s elements using a Galactic chemical evolution (GCE) model, as already discussed by Travaglio et al. (1999, 2001, 2004), with a full updated network and refined asymptotic giant branch (AGB) models. Calculations of the s contribution to each isotope at the epoch of the formation of the solar system is determined by following the GCE contribution by AGB stars only. Then, using the r-process residual method we determine for each isotope their solar system r-process fraction, and recalculate the GCE contribution of heavy elements accounting for both the s and r process. We compare our results with spectroscopic abundances at various metallicities of [Sr,Y,Zr/Fe], of [Ba,La/Fe], of [Pb/Fe], typical of the three s-process peaks, as well as of [Eu/Fe], which in turn is a typical r-process element. Analysis of the various uncertainties involved in these calculations are discussed.

Type
Theory, Evolution and Models
Copyright
Copyright © Astronomical Society of Australia 2009

References

Anders, E. & Grevesse, N. 1989, GeCoA, 53, 197 Google Scholar
Aoki, W. et al., 2005, ApJ, 632, 611 CrossRefGoogle Scholar
Aoki, W. et al., 2006, ApJ, 639, 897 Google Scholar
Aoki, W. et al., 2008, ApJ, 678, 1351 Google Scholar
Aoki, W. & Honda, S. 2008, PASJ, 60, L7 CrossRefGoogle Scholar
Arlandini, C., Käppeler, F., Wisshak, K., Gallino, R., Lugaro, M., Busso, M. & Straniero, O. 1999, ApJ, 525, 886 CrossRefGoogle Scholar
Bao, Z. K., Beer, H., Käppeler, F.,Voss, F.,Wisshak, K. & Rauscher, T., 2000, ADNDT, 76, 70 CrossRefGoogle Scholar
Bisterzo, S., Gallino, R., Straniero, O., Aoki, W., Ryan, S. & Beers, T. C., 2006, AIPC, 847, 368 Google Scholar
Busso, M., Gallino, R. & Wasserburg, G. J. 1999, ARA&A, 37, 239 Google Scholar
Busso, M., Gallino, R., Lambert, D. L., Travaglio, C. & Smith, V. V., 2001, ApJ, 557, 802 Google Scholar
Cescutti, G., François, P., Matteucci, F., Cayrel, R. & Spite, M., 2006, A&A, 448, 557 Google Scholar
Chiappini, C., Matteucci, F. & Gratton, R. 1997, ApJ, 477, 765 Google Scholar
Clayton, D. D. & Rassbach, M. E. 1967, ApJ, 148, 69 Google Scholar
Cohen, J. G., McWilliam, A., Christlieb, N., Shectman, S., Thompson, I., Melendez, J., Wisotzki, L. & Reimers, D. 2007, ApJ, 659, L161 CrossRefGoogle Scholar
Cohen, J. G., Christlieb, N., McWilliam, A., Shectman, S., Thompson, I., Mendelez, J., Wisotzki, L. & Reimers, D. 2008, ApJ, 672, 320 Google Scholar
Cowan, J. J. et al., 2002, ApJ, 572, 861 CrossRefGoogle Scholar
Ferrini, F., Matteucci, F., Pardi, C. & Penco, U. 1992, ApJ, 387, 138 Google Scholar
François, P. et al., 2007, A&A, 476, 935 Google Scholar
Frebel, A., Norris, J. E., Aoki, W., Honda, S., Bessell, M. S., Takada-Hidai, M., Beers, T. C. & Christlieb, N. 2007, ApJ, 658, 534 Google Scholar
Gallino, R., Arlandini, C., Busso, M., Lugaro, M., Travaglio, C., Straniero, O., Chieffi, A. & Limongi, M. 1998, ApJ, 497, 388 Google Scholar
Iben, I. Jr., 1975, ApJ, 196, 525 Google Scholar
Ivans, I. I., Simmerer, J., Sneden, C., Lawler, J., Cowan, J., Gallino, R. & Bisterzo, S. 2006, ApJ, 645, 613 Google Scholar
Käppeler, F., Beer, H., Wisshak, K., Clayton, D. D., Macklin, R. L. & Ward, R. A. 1982, ApJ, 257, 821 Google Scholar
Lai, D. K., Bolte, M., Johnson, J. A., Lucatello, S., Heger, A. & Woosley, S. E. 2008, ApJ, 681, 1524 CrossRefGoogle Scholar
Mashonkina, L. & Zhao, G. 2006, A&A, 456, 313 Google Scholar
Mashonkina, L. et al., 2008, A&A, 478, 529 Google Scholar
Matteucci, F. 2003, ASSL, 253 Google Scholar
Norris, J. E., Christlieb, N., Korn, A. J., Eriksson, K., Bessell, M. S., Beers, T. C., Wisotzki, L. & Reimers, D. 2007, ApJ, 670, 774 Google Scholar
Pagel, B. E. J. 1997, Nucleosyntesis and Chemical Evolution of Galaxies (Cambridge University Press)Google Scholar
Pardi, M. C., Ferrini, F. & Matteucci, F. 1995, ApJ, 444, 207 Google Scholar
Roederer, I. U., Lawler, J. E., Sneden, C., Cowan, J. J., Sobeck, J. & Pilachowski, C. A. 2008, ASPC, 393, 263 Google Scholar
Sneden, C., Cowan, J. J. & Gallino, R. 2008, ARA&A, 46, 241 Google Scholar
Straniero, O., Domínguez, I., Abia, C., Limongi, M. & Chieffi, A., 2001, MmSAI, 72, 265 Google Scholar
Straniero, O., Domínguez, I., Cristallo, S. & Gallino, R. 2003, PASA, 20, 389 Google Scholar
Travaglio, C., Galli, D., Gallino, R., Busso, M., Ferrini, F. & Straniero, O. 1999, ApJ, 521, 691 CrossRefGoogle Scholar
Travaglio, C., Gallino, R., Busso, M. & Gratton, R. 2001, ApJ, 549, 346 Google Scholar
Travaglio, C., Gallino, R., Arnone, E., Cowan, J., Jordan, F. & Sneden, C. 2004, ApJ, 601, 864 Google Scholar
Truran, J. W. & Iben, I. Jr., 1977, ApJ, 216, 797 Google Scholar
Vaglio, P. et al., 1999, in Nuclei in the Cosmos V, Ed. Prantzos, N. (Paris, Edition Frontières), 223 Google Scholar
Van Eck, S., Goriely, S., Jorissen, A. & Plez, B. 2003, A&A, 404, 291 Google Scholar
Wyse, R. F. G. & Gilmore, G. 1992, AJ, 104, 144 Google Scholar
Yushchenko, A. et al., 2005, A&A, 430, 255 Google Scholar