Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-18T18:17:06.125Z Has data issue: false hasContentIssue false

Evolution of Close Binaries

Published online by Cambridge University Press:  14 August 2015

A. V. Tutukov*
Affiliation:
Astronomical Council, USSR Academy of Sciences

Extract

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.

Most stars of our Galaxy's disk are double. The existing estimation of duplicity αα range from ~ 50-70 % (Abt, Levy, 1976, Abt, 1979) to ~ 100 % (Kraitcheva et al., 1978). About half of all stars are close binaries (CB) and hence their components fill their Roche lobes during evolution. This accounts for the constantly increasing interest to their evolution. Several review papers were published in the last years: Paczynski (1971), Tutukov et al. (1975), van den Heuvel (1976), Massevitch et al. (1976), Thomas (1977), Paczynski (1979), Webbink (1979b), Yungelson and Massevitch (1980). The subject matter of close binary evolution is very wide now, therefore, I will limit myself to the review of modern scenarios for evolution of massive (M ≳ 10 M ) close binaries (MCBS) and close binaries of moderate (M ≲ 10 M) mass.

Type
Session 4: Mass Exchange on Close Binary Stars and the Effect on Stellar Evolution
Copyright
Copyright © Reidel 1981 

References

Abt, H.A., Levy, S.G.: 1976, Astrophys. J. Suppl. 30, p.273.Google Scholar
Abt, H.A.: 1979, “The frequency of binaries on the main sequence”, preprint.Google Scholar
Bath, G.T.: 1975, Month. N.R.A.S. 171, p.311.Google Scholar
Binnendijk, L.: 1977, Vistas in Astron. 21, p.359.Google Scholar
Charles, P.: 1980, Sky and Telescope 59, p. 188.Google Scholar
Chiosi, C., Suma, C.: 1970, Astrophys. Sp. Sci. 8, p.478.Google Scholar
Davidson, K., Ostriker, J.P.: 1973, Astrophys. J. 179, p.585.Google Scholar
Fabian, A., Pringle, J., Rees, M.: 1975, Month. N.R.A.S. 172, p.15.Google Scholar
Faulkner, J.: 1974, Proc. IAU Symp. 73, Eds. Eggleton, P., Mitton, S., Wheelan, J., p.193.Google Scholar
Gallagher, J.S., Starrfield, S.: 1978, Ann. Rev. Astron. Astrophys. 16, 171.Google Scholar
Gott, J.R. III: 1972, Astrophys. J. 173, p.227.Google Scholar
Green, R.F., Richstone, D.O., Schmidt, M.: 1978, Astrophys. J. 224, p.892.Google Scholar
Joss, P.C.: 1978, Astrophys. J.L. 225, L123.Google Scholar
Joss, P.C., Rappoport, S.: 1979, Astron. Astrophys. 71, p.217.Google Scholar
Habing, H.J.: 1977, Proc. IAU Coll. 42, Eds. Kippenhahn, R., Rahe, J., Stromeier, W., p.401.Google Scholar
Hanson, R.B.: 1979, Month. N.R.A.S. 186, p.357.Google Scholar
Helfand, D.J., Tademaru, E.: 1977, Astrophys. J. 216, p.842.Google Scholar
Hills, J.G.: 1975, Astron. J. 80, p.809.Google Scholar
Humphreys, R.M., Davidson, K.: 1979, Astrophys. J. 232, p.409.Google Scholar
Hutchings, J.B.: 1975, Astrophys. J. 200, p.122.Google Scholar
Ergma, E.V., Tutukov, A.V.: 1980a, Proc. IAU Symp. 88.Google Scholar
Ergma, E.V., Tutukov, A.V.: 1980b, Proc. IAU Coll. 53.Google Scholar
Kraitcheva, Z.T.: 1974, Nauch. Inform. 31, p.58.Google Scholar
Kraitcheva, Z.T., Popova, E.I., Tutukov, A.V., Yungelson, L.R.: 1978, Astron. Zh. 55, p.1176.Google Scholar
Lebedinsky, A.I., Gurevich, L.E.: 1947, Dokl. Akad. Nauk 55, No.9 (USSR, in Russian).Google Scholar
Lozinskaya, T.A., Tutukov, A.V.: 1980, Nauch. Inform. USSR Acad. Sci., No.49 (in press).Google Scholar
Meyer, F., Meyer-Hoffmeister, E.: 1979, Astron. Astrophys. 78, 167.Google Scholar
Manchester, R.N., Newton, L.M., Cooke, D.J., Lyne, A.G.: 1980, Astrophys. J.L. 236, L25.Google Scholar
Marashi, L., Cavaliere, A.: 1976, Highlights Astron. 4,p.127.Google Scholar
Mason, K.O.: 1977, Month. N.R.A.S. 178, p.81.Google Scholar
Massevitch, A.G., Tutukov, A.V., Yungelson, L.R.: 1976, Astrophys. Sp. Sci. 40, p.115.Google Scholar
Massevitch, A.G., Popova, E.I., Tutukov, A.V., Yungelson, L.R.: 1979, Astrophys. Sp. Sci. 62, p.451.Google Scholar
Massevitch, A.G., Tutukov, A.V.: 1980, “The star evolution”, Moscow (in Russian).Google Scholar
Massevitch, A.G., Tutukov, A.V., Yungelson, L.R.: 1980, Proc. IAU Symp. 93.Google Scholar
Mestel, L.: 1967, Proc. Liège Coll., 1966, p.351.Google Scholar
Mezzetti, M., Ginricin, G., Mardirossian, F.: 1980, Astron. Astrophys. 83, p.217.Google Scholar
Miller, J.S., Krzeminski, W., Priedhorsky, W.: 1976, IAU Circ. No. 2974.Google Scholar
Moffat, A.F.J., Isserstedt, J.: 1979, “The Nature of Single-Line Population I Wolf-Rayet Stars: Evidence for High Space Velocity”, preprint.Google Scholar
Nelson, B., Young, A.: 1970, Publ. Astron. Soc. Pac. 82, p.699.Google Scholar
Osaki, Y.: 1974, Publ. Astron. Soc. Japan 26, p.429.Google Scholar
Paczynski, B.: 1967, Acta Astron. 17, p.355.Google Scholar
Paczynski, B.: 1971, Ann. Rev. Astron. Astrophys. 9, p.183.Google Scholar
Paczynski, B.: 1974, private communication. Google Scholar
Paczynski, B.: 1979a, private communication. Google Scholar
Paczynski, B.: 1979b, review paper at IAU Assembly in Montreal, “Stellar evolution and close binaries”.Google Scholar
Popova, E.I., Tutukov, A.V., Yungelson, L.R.: 1980 (in prep).Google Scholar
Pottasch, S.: 1959, Ann.d'Astrophys., 22, p.412.Google Scholar
Shu, F.H., Lubow, S.H., Anderson, L.: 1979, Astrophys. J. 229, p. 223.Google Scholar
Starrfield, S., Truran, J.W., Sparks, W.M., Kutter, G.S.: 1972, Astrophys. J. 176, p.223.Google Scholar
Starrfield, S.: 1980, Proc. IAU Coll. 53, p.274.Google Scholar
Stone, R.C.: 1979, Astrophys. J. 232, p.520.Google Scholar
Sugimoto, D., Fujimoto, M.Y., Nariai, K., Nomoto, K.: 1980, Proc. IAU Coll. 53.Google Scholar
Svechnikov, M.A.: 1969, Catalog of orbital elements of close binaries, Sverdlovsk.Google Scholar
Taam, R.E., Bodenheimer, P., Ostriker, J.P.: 1978, Astrophys. J. 222, p.269.Google Scholar
Thomas, H.-C.: 1977, Ann. Rev. Astron. Astrophys. 15, p.127.Google Scholar
Thorne, K.S., Zytkow, A.: 1977, Astrophys. J. 212, p.832.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1971, Nauch. Inform. 20,p.86.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1973a, Nauch. Inform. 27,p.58.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1973b, Nauch. Inform. 27,p.70.Google Scholar
Tutukov, A.V., Yungelson, L.R., Kraitcheva, Z.T.: 1975, Mem. Soc. Astron. Ital. 45, p.879.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1976, Astrofizika 12, p.521.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1979a, Proc. IAU Symp. 83.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1979b, Acta Astron. 29, p.665.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1980a, Proc. IAU Symp. 88.Google Scholar
Tutukov, A.V., Yungelson, L.R.: 1980b, Nauch. Inform. 37 (in press).Google Scholar
Vanbeveren, D., Conti, P.S.: 1979, preprint.Google Scholar
Van den Heuvel, E.P.J.: 1968, Bull. Astron. Soc. Nether. 19, p.309.Google Scholar
Van den Heuvel, E.P.J., Heise, J.: 1972, Nat. Phys. Sci. 239, p.67.Google Scholar
Van den Heuvel, E.P.J.: 1976, Proc. IAU Symp. 73, p.35.Google Scholar
Van den Heuvel, E.P.J.: 1980, Proc. of Advanced Study Inst. “Extragalactic X-ray Astronomy”.Google Scholar
Van den Heuvel, E.P.J., Ostriker, J.P., Patterson, J.A.: 1980, Astron. Astrophys. 81, p.7.Google Scholar
Yungelson, L.R.: 1973, Nauch. Inform. 27, p.93.Google Scholar
Yungelson, L.R., Massevitch, A.G.: 1980, “Mass exchange and evolution of close binary stars”, Sov. Sci. Rev., Ed. Syunyaev, R.A. Google Scholar
Ziolkowski, J.: 1977, Ann. New-York Acad. Sci. 302, p.47.Google Scholar
Webbink, R.F.: 1977a, Astrophys. J. 215, p.851.Google Scholar
Webbink, R.F.: 1977b, Proc. IAU Coll. 42, Eds. R. Kippenhahn, Rahe, J., Stromeier, W., p.363.Google Scholar
Webbink, R.F.: 1979a, “The evolutionary significance of recurrent novae”, preprint IAP-79-3, Illinois.Google Scholar
Webbink, R.F.: 1979b, “The formation of white dwarfs in close binary systems”, preprint IAP-79-29, Illinois.Google Scholar
Wheaver, T.A., Woosley, S.E.: 1980, Bull. AAS 12, p.202.Google Scholar
Whelan, J., Iben, I. Jr.: 1973, Astrophys. J. 186, p.1007.Google Scholar
White, C.A., Eggleton, P.P.: 1980, Month. N.R.A.S. 190, p.801.Google Scholar