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Binary S and MS Stars

Published online by Cambridge University Press:  07 August 2017

Hollis R. Johnson
Hollis R. Johnson*
Affiliation:
Astronomy Department SW 319, Indiana University Bloomington, Indiana 47405 U.S.A.

Abstract

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We assemble and discuss evidence for binarity in S and MS stars - stars that are enriched in s-process elements. A popular view is that Tc-deficient S and MS stars are not thermally pulsing AGB stars but are mass-transfer binaries. We describe several methods used to test this hypothesis through a search for the putative white-dwarf companion: (1) periodic radial velocity variations, (2) direct observation of the hot companions with IUE, (3) evidence of a hot gas cloud (hotter than a chromosphere) in the system, and (4) evidence of circumstellar dust as revealed through infrared radiation. Results of these methods are compared. All evidence supports the idea that Tc-deficient S and MS stars are mass-transfer binaries, and a large fraction appear to be interactive.

Type
Invited Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 157 - 166
Copyright
Copyright © Kluwer 1992 

References

Ake, T.B. and Johnson, H.R. 1988, Astrophys. J. 327, 214.Google Scholar
Ake, T.B., Johnson, H.R., and Perry, B.F. 1988, in A Decade of UV Astronomy with IUE, ESA SP-281, p. 245.Google Scholar
Ake, T.B., Johnson, H.R., and Ameen, M.M. 1991, Astrophys. J., in press.Google Scholar
Beavers, W.I. and Eitter, J.J. 1986, Astrophys. J. Suppl. 62, 147.CrossRefGoogle Scholar
Bessell, M.S., Wood, P.R., and Lloyd Evans, T. 1983, Mon. Not. R.A.S. 202, 59.Google Scholar
Brown, J.A., Johnson, H.R., and Hinkle, K.H., 1989, in Evolution of Peculiar Red Giant Stars, ed. Johnson, H.R. and Zuckerman, B. (Cambridge: Cambridge Univ. Press), p. 378.Google Scholar
Brown, J.A., Smith, V.V., Lambert, D.L., Dutchover, E., Hinkle, K.H., and Johnson, H.R. 1990, Astron. J. 99, 1930.CrossRefGoogle Scholar
Frayer, D.T. and Johnson, H.R. 1991, in preparation.Google Scholar
Griffin, R.F. 1984, Observatory 104, 224.Google Scholar
Iben, I. 1987, in Late Stages of Stellar Evolution, ed. Kwok, S and Pottasch, S.R. (Dordrecht: Reidel), p.175.Google Scholar
Iben, I. and Renzini, A. 1983, Ann. Rev. Astr. Ap. 21, 277.CrossRefGoogle Scholar
Johnson, H.R. and Ake, T.B. 1989, in Evolution of Peculiar Red Giant Stars, ed. Johnson, H.R. and Zuckerman, B. (Cambridge: Cambridge Univ Press), p.371.Google Scholar
Johnson, H.R., Ake, T.B., Ameen, M.M., and Brown, J.A. 1989, in From Miras to Planetary Nebulae, ed. Mennessier, M.O. and Omont, A. (Gif sur Yvette: Ed. Frontiers), p. 332.Google Scholar
Johnson, H.R., Ake, T.B., and Ameen, M.M. 1991, Astrophys. J. in preparation.Google Scholar
Jorissen, A. and Mayor, M. 1988, Astron. Astrophys. 198, 187.Google Scholar
Jorissen, A. and Mayor, M. 1991, Astr. Ap., in preparation.Google Scholar
Jura, M. 1986, Publ. Irish Astron. Soc. 17, 322 Google Scholar
Jura, M. 1988, Astrophys. J. Suppl., 66, 33.CrossRefGoogle Scholar
Kenyon, S.J. 1986, The Symbiotic Stars (Cambridge: Cambridge Univ. Press), p. 115.CrossRefGoogle Scholar
Lambert, D.L. 1987, Astrophys. J. Suppl. 65, 255.Google Scholar
Lambert, D.L. 1991, in The Photospheric Abundance Connection, ed. Michael, G. and Tutukov, A. (Dordrecht: Kluwer), p. 299.Google Scholar
Lattanzio, J.C. 1989, in Evolution of Peculiar Red Giant Stars, ed. Johnson, H.R. and Zuckerman, B. (Cambridge: Cambridge Univ. Press), p.161.Google Scholar
Little, S.J., Little-Marinen, I.R., and Bauer, W.H. 1987, Astron. J. 94, 987 (LLB).Google Scholar
Little-Marenin, I.R. 1989, in Evolution of Peculiar Red Giant Stars, ed. Johnson, H.R. and Zuckerman, B. (Cambridge: Cambridge Univ. Press) p. 131.Google Scholar
Little-Marenin, I.R. and Little, S.J. 1979, Astron. J. 84, 1374.Google Scholar
Lloyd Evans, T. 1984, Mon. Not. R.A.S. 208, 447.Google Scholar
McClure, R.D., Fletcher, J.M., and Nemec, J.M. 1980, Astrophys. J. Lett. 238, L35.CrossRefGoogle Scholar
McClure, R.D. and Woodsworth, A.W. 1991, Astrophys. J. 280, L31.CrossRefGoogle Scholar
Merrill, P. 1952, Astrophys. J. 116, 21.CrossRefGoogle Scholar
Peery, B.F. 1985, in Cool Stars with Excesses of Heavy Elements, ed. Jaschek, M. and Keenan, P.C. (Dordrecht: Reidel), p. 333.Google Scholar
Peery, B.F. 1986, in New Insights in Astrophysics: 8 Years of UV Observations with IUE, ed. Rolfe, E.J., ESA SP-263, p.117.Google Scholar
Scalo, J.M. and Miller, G.E. 1981, Astrophys. J. 246, 251 CrossRefGoogle Scholar
Shcherbakov, A.G. 1979, Sov. Astron. Lett. 5, 290.Google Scholar
Smith, V.V. and Lambert, D.L. 1985, Astrophys. J. 294, 326.Google Scholar
Smith, V.V. and Lambert, D.L. 1986, Astrophys. J. 311, 843.Google Scholar
Smith, V.V. and Lambert, D.L. 1987, Astron. J. 94, 977.Google Scholar
Smith, V.V. and Lambert, D.L. 1988, Astrophys. J. 333, 219.Google Scholar
Smith, V.V. and Lambert, D.L. 1990, Astrophys. J. Suppl. 72, 387.Google Scholar
van der Veen, W.E.C.J., and Habing, H. 1988, Astron. Astrophys. 194, 125.Google Scholar
Walker, H.J. and Cohen, M. 1988, Astron. J. 95, 1801.CrossRefGoogle Scholar
Wing, R.F. and Yorka, S.B. 1977, Mon. Not. R.A.S. 178, 383.Google Scholar
Wood, P.R. 1985, in Cool Stars with Excesses of Heavy Elements, ed. Jaschek, M. and Keenan, P.C. (Dordrecht: Reidel), p. 357.Google Scholar
Zirin, H. 1986, Astrophys. J. 208, 414.Google Scholar
Zirin, H. 1982, Astrophys. J. 260, 655.CrossRefGoogle Scholar