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Abundances in Cool Evolved Stars

Published online by Cambridge University Press:  12 April 2016

Catherine A. Pilachowski
Catherine A. Pilachowski*
Affiliation:
National Optical Astronomy Observatories, Kitt Peak National Observatory PO Box 26732, Tucson, AZ 85726-6732, USA

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Nature has filled the upper right quadrant of the Hertzsprung-Russell diagram with more varieties of peculiar stars and odd chemical compositions than even our most speculative observers and theorists could dream up. To bring some structure to this vast subject I will categorize the phenomena we observe according to our model of stellar evolution, dividing the stars among the first ascent of the giant branch and the core-helium burning phase, the asymptotic giant branch (double shell-burning) phase, and the post-AGB and pre-planetary nebula stars. The types of stars found in these three groups are summarized below.

Type
Part I. Chemical Peculiarities as Probe of Stellar Evolution
Information
International Astronomical Union Colloquium , Volume 108: Atmospherics Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion , 1988 , pp. 17 - 30
Copyright
Copyright © Springer-Verlag 1988

References

Boesgaard, A.M. 1970, Ap. J., 161, 1003.CrossRefGoogle Scholar
Bond, H.E. and Luck, R.E. 1987b, “Proceedings of the ESO Workshop on Stellar Evolution and Dynamics in the Outer Halo of the Galaxy,” April, 1987; Garching.Google Scholar
Brown, J.A. 1987, Ap. J., 317, 701.Google Scholar
Catchpole, R.M. and Feast, M.W. 1971, M.N.R.A.S., 154, 197.Google Scholar
Cowley, C.R. and Downs, P.L. 1980, Ap. J., 236, 648.CrossRefGoogle Scholar
Dearborn, D.S.P., Eggleton, P.E., and Schramm, D.N. 1976, Ap. J., 203, 455.Google Scholar
Dominy, J.F. 1984, Ap. J. Suppl., 55, 27.CrossRefGoogle Scholar
Dominy, J.F. and Wallerstein, G. 1987, Ap. J., 317, 810.Google Scholar
Dominy, J.F., Wallerstein, G., and Suntzeff, N.B. 1986, Ap. J., 300, 325.Google Scholar
Fujita, Y. and Tsuji, T. 1965, Publ. Dom. Astro. Obs., 12, 339.Google Scholar
Fujita, Y. and Tsuji, T. 1977, P.A.S.J., 29, 711.Google Scholar
Hinkle, K.H. and Scharlach, W.W.G. 1985, in “Cool Stars with Excesses of Heavy Elements,” Jaschek, M. and Keenan, P.C., eds.; Dordrecht: Reidel, pp. 255–261.Google Scholar
Harris, M.J. and Lambert, D.L. 1984, Ap. J., 285, 674.Google Scholar
Harris, M.J., Lambert, D.L., Hinkle, K.H., Gustafsson, B., and Eriksson, K. 1987, Ap. J., 316, 294.Google Scholar
Harris, M.J., Lambert, D.L., and Smith, V.V. 1985a, Ap. J., 292, 620.Google Scholar
Harris, M.J., Lambert, D.L., and Smith, V.V. 1985b, Ap. J., 299, 375.Google Scholar
Iben, I. and Renzini, A. 1984, Phys. Letters, 105, 329.Google Scholar
Iben, I. and Tutukov, A.V. 1985, Ap. J. Suppl., 58, 661.Google Scholar
Johnson, H.K., O’Brien, G.T., and Climenhaga, J.C. 1982, Ap. J., 254, 175.Google Scholar
Jura, M. 1986, Ap. J., 309, 732.Google Scholar
Kovacs, N. 1985, Astron. Ap., 150, 232.Google Scholar
Krishnaswamy, K. and Sneden, C. 1984, P.A.S.P., 97, 407.Google Scholar
Lambert, D.L. 1985, in “Cool Stars with Excesses of Heavy Metals,” Jaschek, M. and Keenan, P.C., eds.; Dordrecht: Reidel; pp. 191–219.Google Scholar
Lambert, D.L. 1986, in “Hydrogen Deficient Stars and Related Objects,” Hunger, K., Schonberner, D., and Rao, N.K., eds.; Dordrecht: Reidel; pp. 127–150.CrossRefGoogle Scholar
Lambert, D.L. and Dominy, J.F. 1980, Ap. J., 235, 114.Google Scholar
Lambert, D.L., Gustafsson, B., Eriksson, K., Hinkle, K.H. 1986, Ap. J. Suppl., 62, 373.CrossRefGoogle Scholar
Lambert, D.L. and Ries, L.M. 1981, Ap. J., 248, 228.Google Scholar
Lambert, D.L. and Sawyer, S.R. 1984, Ap. J., 283, 192.CrossRefGoogle Scholar
Luck, R.E. 1982, P.A.S.P., 94, 811.Google Scholar
Luck, R.E. and Bond, H.E. 1982, Ap. J., 259, 792.Google Scholar
Luck, R.E. and Sneden, C. 1986, P.A.S.P., 98, 320.Google Scholar
Little-Marenin, I. and Little, S. 1979, A. J., 84, 1374.Google Scholar
Lloyd Evans, T. 1986, M.N.R.A.S., 220, 723.Google Scholar
McCabe, E.M., Connon Smith, R., and Clegg, R.E.S. 1979, Nature, 281, 263.Google Scholar
McClure, R.D. 1985, in “Cool Stars with Excesses of Heavy Metals,” Jaschek, M. and Keenan, P.C., eds.; Dordrecht: Reidel, pp. 315 – 330.Google Scholar
Merrill, P.W. 1952, Ap. J., 116, 21.Google Scholar
Parthasarathy, M., Sneden, C., and Bohm-Vitense, E. 1984, P. A. S. P., 96, 44.CrossRefGoogle Scholar
Pinsonneault, M.H., Sneden, C., and Smith, V.V. 1984, P.A.S.P., 96, 239.Google Scholar
Schwarzschild, M. and H*:arm, R. 1965, Ap. J., 142, 855.CrossRefGoogle Scholar
Smith, V.V. 1984, Astron. Ap., 132, 326.Google Scholar
Smith, V.V. and Lambert, D.L. 1985, Ap. J., 294, 326 Google Scholar
Smith, V.V. and Lambert, D.L. 1986, Ap. J., 311, 843.Google Scholar
Sneden, C. 1983, P.A.S.P., 95, 745.Google Scholar
Sneden, C. and Bond, H. 1976, Ap. J., 204, 810.Google Scholar
Sneden, C., Lambert, D.L., and Pilachowskl, C.A. 1981, Ap. J., 247, 1052.Google Scholar
Sneden, C. and Pilachowski, C.A. 1984, P.A.S.P., 96, 38.CrossRefGoogle Scholar
Sneden, C., Pilachowski, C.A., and VandenBerg, D.A. 1986, Ap. J., 311, 826.Google Scholar
Tomkin, J., Sneden, C., and Cottrell, P.L. 1984, P.A.S.P., 96, 609.CrossRefGoogle Scholar
Torres-Peimbert, S. and Wallerstein, G. 1966, Ap. J., 146, 724.Google Scholar
Tsuji, T. 1985, in “Cool Stars with Excesses of Heavy Elements,” Jaschek, M. and Keenan, P.C., eds., Dordrecht: Reidel, pp. 295–300.Google Scholar
Tsuji, T. 1986, Astron. Ap., 156, 8.Google Scholar
Utsumi, K. 1985, in “Cool Stars with Excesses of Heavy Elements,” Jaschek, M. and Keenan, P.C., eds., Dordrecht: Reidel, pp. 243–247.Google Scholar
Utsumi, K. 1988, this volume.Google Scholar
Walker, H.J. 1986, in “Hydroden Deficient Stars and Related Objects,” Hunger, K., Schonberner, D., and Rao, N.K., eds.; Dordrecht: Reidel; pp. 407–419.Google Scholar
Wallerstein, G. and Sneden, C. 1982, Ap. J., 255, 577.CrossRefGoogle Scholar
Wannier, P.G. 1985, Proceedings of the ESO Workshop on “Production and Distribution of C, N, 0 Elements,” Garching, pp. 233-247.Google Scholar
Webbink, R.F. 1984, Ap. J., 277, 355.CrossRefGoogle Scholar
Yamashita, Y. 1972, Ann. Tokyo Astron. Obs., 13, 169.Google Scholar
Yamashita, Y. 1975, P. A. S. J., 27, 325.Google Scholar
Zook, A.C. 1985, Ap. J., 289, 356.Google Scholar