Hostname: page-component-669899f699-rg895 Total loading time: 0 Render date: 2025-05-03T19:51:07.649Z Has data issue: false hasContentIssue false
  • English
  • Français

The Formation and Evolution of Low-Mass Close Binaries with Compact Components

Published online by Cambridge University Press:  12 April 2016

A.V. Tutukov  and
L.R. Yungelson
A.V. Tutukov
Affiliation:
Astronomical Council of the USSR Academy of Sciences, Moscow, U.S.S.R.
L.R. Yungelson
Affiliation:
Astronomical Council of the USSR Academy of Sciences, Moscow, U.S.S.R.

Abstract

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.

We discuss the formation and evolution of interacting low-mass close binaries with a He-ICO- or ONe-dwarf neutron star or a black hole as a compact component. Mass exchange leads to cataclysmic events in such systems. The rate of semidetached low-mass close binary formation is 5×10−3 yr−1 if the accreting component is a He degenerate dwarf, 5×10−3 yr−1 if it is a CO-dwarf and 3×10−8 yr−1 if it is a neutron star. Systems with compact accretors arise as the result of the common envelope phase of close binary evolution or due to collisions of single neutron stars or dwarfs with low-mass single stars in dense stellar clusters. Evolution of LMCB to the contact phase in semi-detached stages is determined mainly by the angular momentum losses by a magnetic stellar wind and radiation of gravitational waves. Numerical computations of evolution with momentum loss explain observed mass exchange rates in such systems, the absence of cataclysmic variables with orbital periods 2h−3h, the low number and the evolutionary status of systems with orbital periods shorter than 80m. In conclusion we list unsolved problems related to magnetic stellar wind, the distribution of young close binaries over main initial parameters, stability of mass exchange.

Type
I. Evolution
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 15 - 33
Copyright
Copyright © Reidel 1987

References

Bath, G.T., 1975, Mon. Not. R. Astron. Soc., 171, 311.Google Scholar
Bond, H.E., 1985, in Cataclysmic Variables and Low-Mass X-Ray Binaries, ed. Lamb, D.Q. and Patterson, J. (Reidel, Dordrecht), p. 15.Google Scholar
Cannizzo, J.K., Wheeler, J.C. and Ghosh, P., 1985, in Cataclysmic Variables and Low-Mass X-Ray Binaries, ed. Lamb, D.Q. and Patterson, J. (Reidel, Dordrecht), p. 307.Google Scholar
Edwards, D.A., 1985, Mon. Not. R. Astron. Soc., 212, 623.Google Scholar
Fabian, A.C., Pringle, F.E. and Rees, M.J., 1975, Mon. Not. R. Astron. Soc., 172, 15.Google Scholar
Fedorova, A.V. and Yungelson, L.R., 1984, Space Sci., 103, 125.Google Scholar
Gurevich, A.L. and Lebedinskij, M.A., 1947, Zh. Eksper. i Teor. Fiz., 17, 792 (in Russian).Google Scholar
Hertz, P. and Grindlay, J.E., 1983, Ap. J., 275, 105.Google Scholar
Hertz, P. and Wood, K.S., 1985, Ap. J., 290, 171.Google Scholar
Hills, T.G., 1975, Astron. J., 80, 809.Google Scholar
Hut, P., Paczynski, B., 1984, Ap. J., 284, 675.Google Scholar
Iben, I. Jr., and Tutukov, A.V., 1984a, Ap. J., 284, 719 Google Scholar
Iben, I. Jr., and Tutukov, A.V., 1984b, in High Energy Transients in Astrophysics, ed. Woosley, S.E. (Amer. Inst. Phys., New-York).Google Scholar
Iben, I. Jr., and Tutukov, A.V., 1985, Ap. J. Suppl., 58, 611.Google Scholar
Kraft, P.P., Mathews, J. and Greenstein, J.L., 1962, Ap. J., 136, 312.Google Scholar
Kraicheva, Z.T., Tutukov, A.V. and Yungelson, L.R., 1986, Astrofizika, in press.Google Scholar
MacDonald, T., 1984, Ap. J., 283, 241.Google Scholar
Maraschi, L. and Cavaliere, A., in Highlights of Astronomy, 4, ed. Müller, E.A., p. 127.Google Scholar
Meyer, F. and Meyer-Hoffmeister, E., 1979, Astron.Ap. 78, 167.Google Scholar
Osaki, Y., 1974, Publ.Astron.Soc.Japan, 26, 429.Google Scholar
Paczynski, B., 1976, Structure and Evolution of Close Binary Systems, ed. Eggleton, P. (Reidel, Dordrecht), p. 75.Google Scholar
Paczynski, B., 1981, Acta Astron., 21, 4.Google Scholar
Paczynski, B., 1985, in Cataclysmic Variables and Low-Mass X-Ray Binaries, Eds. Lamb, D.Q., Patterson, J. (Reidel, Dordrecht, p.1).Google Scholar
Patterson, J., 1984, Ap. J. Suppl., 54, 443.Google Scholar
Popova, E.I., Tutukov, A.V. and Yungelson, L.R., 1982, Ap. Space Sci, 88, 155.Google Scholar
Rappaport, S., Verbunt, F. and Joss, P.C., 1983, Ap. J., 275, 713.Google Scholar
Ritter, H., 1984, Preprint MPA-106.Google Scholar
Ritter, H. and Bunkert, A., 1985, in Recent Results on Cataclysmic Variables, Bamberg, p. 17.Google Scholar
Ruderman, M.A. and Shaham, T., 1983, Nature 304, 425.Google Scholar
Savonije, G.I., deKool, M. and van den Heuvel, E.P.J., 1986, Astron. Ap., 155, 51.Google Scholar
Skumanich, A., 1972, Ap. J., 171, 561.CrossRefGoogle Scholar
Spruit, H.C. and Ritter, H., 1983, Astron. Ap., 121, 267 Google Scholar
Taam, R.E. and Wade, R.A., 1985, Ap. J., 293, 504.Google Scholar
Tutukov, A.V., Yungelson, L.R. and Klayman, Ya., 1973, Nauchn. Inform., 27, 3 Google Scholar
Tutukov, A.V. and Yungelson, L.R., 1979a, Acta Astron., 29, 665.Google Scholar
Tutukov, A.V. and Yungelson, L.R., 1979b, in Mass Loss and Evolution of O-type stars, Eds. Conti, P.S. and de Loore, , Reidel, Dordrecht, p. 216.Google Scholar
Tutukov, A.V. and Yungelson, L.R., 1981, Nauchn. Inform., 49, 3.Google Scholar
Tutukov, A.V. and Yungelson, L.R., 1985, in Recent Results on Cataclysmic Variables, Bamberg p. 7.Google Scholar
Tutukov, A.V. and Yungelson, L.R., 1985, Nauchn. Inform, (in press).Google Scholar
Tutukov, A.V., Fedorova, A.V., Yungelson, L.R., 1982, Pis’ma Astron. Zh., 8, 365 Google Scholar
Tutukov, A.V., Fedorova, A.V., Ergma, E.V. and Yungelson, L.R., 1985, Pis’ma Astron. Zh., 11, 23.Google Scholar
Tutukov, A.V., Fedorova, A.V., Ergma, E.V. and Yungelson, L.R., 1986a, Astrofizika, 24, 85.Google Scholar
Tutukov, A.V., Fedorova, A.V. and Yungelson, L.R., 1986b, Nauchn. Inform, (in press).Google Scholar
Tutukov, A.V., 1981, in Fundamental Problems in Stellar Evolution, eds. Sugimoto, D., Lamb, D.Q., Schramm, D.N. (Reidel, Dordrecht), p. 116.Google Scholar
Tutukov, A.V., 1983, Preprint of Illinois Univ., IAP 83-25.Google Scholar
Verbunt, F., 1981, Mon. Not. R. Astron. Soc., 209, 227.Google Scholar
Verbunt, F. and Zwaan, C., 1981, Astron. Ap., 100. L7.Google Scholar
Webbink, R.F., 1985, preprint.Google Scholar
Whelan, J.A.J. and Iben, I. Jr., 1983, Ap. J., 186, 1007.Google Scholar
Yungelson, L.R. and Massevitch, A.G., 1983, Soviet Sci. Revs., Astrophys. and Space Phys. Revs., ed. Syunyaev, R., 2, P. 29.Google Scholar