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The Barium Stars

Published online by Cambridge University Press:  07 August 2017

Verne V. Smith
Verne V. Smith*
Affiliation:
Department of Astronomy and McDonald Observatory The University of Texas Austin, TX 78712 USA

Abstract

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The Barium stars are reviewed in terms of their known binary nature and their quantitative abundance peculiarities. It is concluded that the most likely explanation of the 12C and s-process overabundances observed in the Barium stars is mass transfer from a companion, which is now a white dwarf, but was once a 4He-burning thermally-pulsing asymptotic giant branch star.

Type
Invited Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 103 - 113
Copyright
Copyright © Kluwer 1992 

References

Bidelman, W. P., and Keenan, P. C. 1951, Ap. J. , 114, 473.Google Scholar
Boffin, H. M. J. 1992 - this volume.Google Scholar
Boffin, H. M. J., and Jorissen, A. 1988, A&A , 205, 155.Google Scholar
Böhm-Vitense, E. 1980, Ap. J. , 239, L79.CrossRefGoogle Scholar
Böhm-Vitense, E., Nemec, J. M., and Proffitt, C. 1984, Ap. J. , 278, 726.CrossRefGoogle Scholar
Bond, H. E. 1974, Ap. J. , 194, 95.CrossRefGoogle Scholar
Bond, H. E. 1984, in Future of UV Astronomy Based on Six Years of IUE Research , NASA Conf. Publ. No. 2349, p. 289.Google Scholar
Burbidge, E. M., and Burbidge, G. R. 1957, Ap. J. , 126, 357.Google Scholar
Burbidge, E. M., Burbidge, G. R., Fowler, W. A., and Hoyle, F. 1957, Rev. Mod. Phys. , 29, 547.CrossRefGoogle Scholar
Dominy, J. F., and Lambert, D. L. 1983, Ap. J. , 270, 180.Google Scholar
Dominy, J. F., Wallerstein, G., and Suntzeff, N. B. 1986, Ap. J. , 300, 325.Google Scholar
Garstang, R. H. 1952, PASP , 93, 641.CrossRefGoogle Scholar
Griffin, R. F. 1983, Observatory , 103, 273.Google Scholar
Griffin, R. F. 1984a, Observatory , 104, 6.Google Scholar
Griffin, R. F. 1984b, Obervatory , 104, 268.Google Scholar
Griffin, R. F. 1985a, Observatory , 105, 9.Google Scholar
Griffin, R. F. 1985b, Observatory , 105, 128.Google Scholar
Griffin, R. F. 1985c, in Interacting Binaries , ed. Eggleton, P. P. and Pringle, J. E. (Dordrecht: Reidel), p. 1.Google Scholar
Griffin, R. F. 1986a, Observatory , 106, 35.Google Scholar
Griffin, R. F. 1986b, Observatory , 106, 108.Google Scholar
Griffin, R. F. 1988a, Observatory , 108, 17.Google Scholar
Griffin, R. F. 1988b, Observatory , 108, 90.Google Scholar
Iben, I. Jr. 1975, Ap. J. , 196, 549.CrossRefGoogle Scholar
Iben, I. Jr., and Truran, J. W. 1978, Ap. J. , 220, 980.CrossRefGoogle Scholar
Iben, I. Jr., and Renzini, A. 1983, ARAA , 21, 271.Google Scholar
Johnson, J. R. 1992 - this volume.Google Scholar
Jorissen, A., Smith, V. V., and Lambert, D. L. 1992, A&A , in press.Google Scholar
Keenan, P. C. 1942, Ap. J. , 96, 101.Google Scholar
Kovacs, N. 1985, A&A , 150, 232.Google Scholar
Krishnaswamy, K., and Sneden, C. 1985, PASP , 97, 407.CrossRefGoogle Scholar
Lambert, D. L. 1985, in Cool Stars with Excesses of Heavy Elements , ed. Jaschek, M. and Keenan, P. C. (Dordrecht: Reidel), p. 191.CrossRefGoogle Scholar
Lambert, D. L. 1988, in The Impact of Very High S/N Spectroscopy on Stellar Physics , ed. de Strobel, G. Cayrel and Spite, M. (Dordrecht: Kluwer), p. 563.CrossRefGoogle Scholar
Lambert, D. L., and Ries, L. M. 1981, Ap. J. , 248, 228.CrossRefGoogle Scholar
Lambert, D. L., Gustafsson, B., Eriksson, K., and Hinkle, K. H. 1986, Ap. J. Suppl. , 62, 373.CrossRefGoogle Scholar
Little, S. J., Little-Marenin, I. R., and Bauer, W. H. 1987, A. J. , 94, 981.Google Scholar
Luck, R. E., and Bond, H. E. 1982, Ap. J. , 259, 792.Google Scholar
Luck, R. E. 1991, Ap. J. , in press.Google Scholar
MacConnell, F. J., Frye, P. L., and Upgren, A. R. 1972, A. J. , 77, 384.Google Scholar
McClure, R. D. 1983, Ap. J. , 268, 264.CrossRefGoogle Scholar
McClure, R. D. 1984a, PASP , 96, 117.CrossRefGoogle Scholar
McClure, R. D. 1984b, Ap. J. , 280, L31.CrossRefGoogle Scholar
McClure, R. D. 1989, in Evolution of Peculiar Red Giants , ed. Johnson, H. R. and Zuckerman, B. (Cambridge: Cambridge University Press), p. 101.Google Scholar
McClure, R. D., and Woodsworth, A. W. 1990, Ap. J. , 352, 709.Google Scholar
McClure, R. D., Fletcher, J. M., and Nemec, J. M. 1980, Ap. J. , 238, L35.Google Scholar
North, P., and Duquennay, A. 1990, in Stellar Evolution: The Photospheric Abundance Connection , ed. Michaud, G. (Dordrecht: Kluwer), p. —.Google Scholar
Sanders, R. H. 1967, Ap. J. , 150, 971.Google Scholar
Scalo, J. M. 1976, Ap. J. , 206, 474.CrossRefGoogle Scholar
Schwarzschild, M., and Härm, R. 1967, Ap. J. , 150, 961.Google Scholar
Smith, V. V. 1984, A&A , 132, 326.Google Scholar
Smith, V. V., and Lambert, D. L. 1988, Ap. J. , 333, 219.CrossRefGoogle Scholar
Smith, V. V. 1990, Ap. J. Suppl. , 72, 387.Google Scholar
Smith, V. V., Sneden, C., and Pilachowski, C. A. 1980, PASP , 92, 809.Google Scholar
Smith, V. V., Coleman, H., and Lambert, D. L. 1992, Ap. J. , submitted.Google Scholar
Sneden, C. 1983, PASP , 95, 745.CrossRefGoogle Scholar
Sneden, C., and Bond, H. E. 1976, Ap. J. , 204, 810.Google Scholar
Sneden, C., Lambert, D. L., and Pilachowski, C. A. 1981, Ap. J. , 247, 1052.Google Scholar
Tech, J. 1971, NBS Monograph 61 (Washington, D.C.: Government Printing Office).Google Scholar
Tomkin, J., and Lambert, D. L. 1979, Ap. J. , 227, 209.Google Scholar
Tomkin, J., Lambert, D. L., Edvardsson, B., Gustafsson, B., and Nissen, P. E. 1989, A&A , 219, L15.Google Scholar
Utsumi, K. 1985, in Cool Stars with Excesses of Heavy Elements , ed. Jashek, M. and Keenan, P. C. (Dordrecht: Reidel), p. 243.Google Scholar
Warner, B. 1965, MNRAS , 129, 263.Google Scholar
Webbink, R. F. 1986, in Critical Observations versus Physical Models for Close Binary Systems , ed. Leung, K.-C. and Zhai, D. S. (New York City: Gordon and Breach), p. 403.Google Scholar