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Stellar Evolution and Close Binaries

Published online by Cambridge University Press:  30 March 2016

B. Paczynski
B. Paczynski*
Affiliation:
N. Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warazawa, Poland

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A general scheme of evolution of close binaries is outlined. Many types of observed systems are classified according to their evolutionary status. Present theory can account reasonably well for the mass transfer between the two components. There is no satisfactory theory of mass and angular momentum loss from binary (as well as single) stars. Most close binaries sooner or later should develop extended common envelopes. A loss of a common envelope may remove a large fraction of mass and most of angular momentum from a binary, and leave as a remnant a very short period and highly evolved system. Binary nuclei of planetary nebulae, cataclysmic variables and some X-ray binaries are produced this way.

I shall present here a picture of the evolution of close binary systems (CBS) as it is understood now. This is not intended to be a review, and no attempt has been made to make the list of references complete. Usually I shall refer the first paper on a given subject and/or one of the recent ones, where a large number of other references can be found. There are many reviews and proceedings of various symposia that deal with close binaries. Here are some: Annual Review of Astronomy and Astrophysics (9, 183, 14, 119, 15, 127, 16, 171, 241), IAU Symposia No. 73, 83, 88, IAU Colloquia No. 42, 46, 53. I shall try to emphasize what is known and what is not known, and how various observed systems fit into the theoretical evolutionary scheme. Because of my background I shall give more references to theoretical papers. Nevertheless, I am convinced that it was the theory of close binaries that was guided in its development by the observations, not other way around. In fact the theory predicted very few new phenomena and very few new types of binaries. But it managed to account, at least qualitatively, for the major evolutionary processes, and made it possible to arrange the observed systems into the evolutionary sequences.

Type
Invited Discourses & A Selected Paper
Information
Highlights of Astronomy , Volume 5: Highlights of Astronomy. As presented at the XVIIth General Assembly of the IAU, 1979 , 1980 , pp. 27 - 44
Copyright
Copyright © Cambridge University Press 1980

References

Abt, H.A., and Levy, S.G., 1976. Astrophys. J. Suppl., 30., 273.Google Scholar
Abt, H.A., and Levy, S.G., 1978. Astrophys. J. Suppl., 36, 241.Google Scholar
Acker, A., 1978. IAU Symp. No. 76, p. 209, Terzian, Y. (ed).Google Scholar
Bath, G.T., 1973. Nature Phys. Sci., 246, 84.CrossRefGoogle Scholar
Begelman, M.C., 1978. Monthly Not. Royal Astron. Soc., 184., 53.Google Scholar
Benson, R.S., 1970. Ph.D. Thesis, Univ. of Calif., Berkeley.Google Scholar
Bond, H.E., Liller, W., and Mannery, E.J., 1978. Astrophys. J., 223, 252.Google Scholar
Cameron, A.G.W., and Mock, M., 1967. Nature, 215, 464.Google Scholar
Clark, G.W., 1975. Astrophys. J., 199, L143.Google Scholar
Cowley, A.P., Crampton, D., and Hutchings, J.B., 1979. Astrophys. J., 231, 539.Google Scholar
Crawford, J.A., 1955. Astrophys. J., 121, 71.Google Scholar
DeCampli, W.M., and Baliunas, S.L., Astrophys. J., 230, 815.Google Scholar
Dworetsky, M.M., Lanning, H.H., Etzel, P.B., and Patenaude, D.J., 1977. Monthly Not. Royal Astron. Soc., 181, 13P.Google Scholar
Fabian, A., Pringle, J., and Rees, M., 1975. Monthly Not. Royal Astron. Soc., 172, 15P.Google Scholar
Flannery, B., and Ulrich, R., 1977. Astrophys. J., 212, 533.Google Scholar
Guy Morgan, J., and Eggleton, P.P., 1979. Monthly Not. Royal Astron. Soc., 187, 661.Google Scholar
Hall, D.S., 1979. Preprint, to be published in Acta Astron Jaroszynski, M., Abramowicz M.A., and Paczynski, B. 1979.Google Scholar
Johnson, H.L. and Sandage, A.R., 1956. Astrophys. J., 124, 379.Google Scholar
Joss, P.C., and Rappaport, S., 1079. Astron. Astrophys., 71, 217.Google Scholar
Kippenhahn, R., and Meyer-Hofmeister, E., 1977. Astron. Astrophys., 54, 539.Google Scholar
Kippenhahn, R., Thomas, H.C., and Weigert, A., 1968. Zeit. Astrophys., 69, 265.Google Scholar
Kippenhahn, R., and Weigert, A., 1968. Zeit. Astrophys., 65, 251.Google Scholar
Kreiner, J.M., and Ziolkowski, J., 1978. Acta Astron., 28, 497.Google Scholar
Kruszewski, A., 1963. Acta Astron., 13, 106.Google Scholar
Kruszewski, A., 1967. Acta Astron., 17, 297.Google Scholar
Kuiper, G.P., 1941. Astrophys. J., 93, 133.Google Scholar
Lewin, W.H.G., and Clark, G.W., 1978. Presented at 9th Texas Symposium, Munich, December 1978.Google Scholar
Lin, D.N.C., and Papaloizou, J., 1979a. Monthly Not. Royal Astron. Soc., 186, 799.Google Scholar
Lin, D.N.C., and Papaloizou, J., 1979b. Monthly Not. Royal Astron. Soc., 188, 191.Google Scholar
Lubow, S.H., and Shu, F.H., 1975. Astrophys. J., 198, 383.Google Scholar
Lucy, L.B., and Wilson, R.E., 1979. Astrophys. J., 231, 502.Google Scholar
Lutz, J., 1978. IAU Symp. No. 76, p. 185, Terzian, Y. (ed).Google Scholar
Lynden-Bell, D., and Pringle, J.E., 1974. Monthly Not. Royal Astron. Soc., 168, 603.Google Scholar
Massevitch, A.G., Tutukov, A.V., and Yungelson, L.R., 1976. Astrophys. Space Sci., 40, 115.Google Scholar
McCrea, W.H., 1964. Monthly Not. Royal Astron. Soc., 128, 147.CrossRefGoogle Scholar
Mestel, L., 1967. Proceedings, Liege Colloquium 1966, p. 351.Google Scholar
Meyer, F., and Meyer-Hofmeister, E., 1979. Astron. Astrophys., in press.Google Scholar
Milgrom, M., 1978. Astron. Astrophys., 67, L25.Google Scholar
Miller, J.S., Krzeminski, W., and Priedhorsky, W., 1976. IAU Circ., No. 2974.Google Scholar
Morton, D.C., 1960. Astrophys. J., 132, 146.Google Scholar
Nakamura, Y.- Saio, H., and Sugimoto, D., 1978. Publ. Astron. Soc. Japan, 30, 649.Google Scholar
Nelson, B., and Young, A., 1970. Publ. Astron. Soc. Pacific, 82, 699.Google Scholar
Neo, S., Miyaji, S., Nomoto, K., and Sugimoto, D., 1977. Publ. Astron. Soc Japan, 29, 249.Google Scholar
Osaki, Y., 1974. Publ. Astron. Soc. Japan, 26, 429.Google Scholar
Paczynski, B., 1966. IAU Colloquium No. 6, p. 139, Gyldenkerne, K. R. M. West (eds).Google Scholar
Paczynski, B., 1967 Acta Astron., 17, 287.Google Scholar
Paczynski, B., 1967b. Acta Astron., 17, 355.Google Scholar
Paczynski, B., 1976. IAU Symp. No. 73, p. 75, Eggleton, P. et al. (eds).Google Scholar
Paczynski, B., 1977. Astrophys. J., 216, 822.Google Scholar
Paczynski, B., and Rudak, B., 1979. Astron. Astrophys., in press.Google Scholar
Paczynski, B., and Sienkiewicz, R., 1972. Acta Astron., 22, 73.Google Scholar
Paczynski, B., and Wiita, P.J., 1978. Submitted to Astron. Astrophys.Google Scholar
Paczynski, B., and Zytkow, A., 1978. Astrophys. J., 222, 604.Google Scholar
Papaloizou, J., and Pringle, J.E., 1977. Monthly Not. Royal Astron. Soc., 181, 441.Google Scholar
Patterson, J., 1979. Preprint.Google Scholar
Plavec, M., 1958. 8th Liege Colloquium, Mem. 8 Soc. Royal Sci. Liege, 4th Ser., 20, 411.Google Scholar
Popper, D., 1973. Astrophys. J., 185, 265.Google Scholar
Prendergast, K.H., and Burbidge, G.R., 1968, Astrophys. J., 151, L83.Google Scholar
Pringle, J.E., and Rees, M.J., 1972. Astron. Astrophys. 21, 1.Google Scholar
Refsdal, S., Roth, M.L., and Weigert, A., 1974. Astron. Astrophys., 36, 113.Google Scholar
Ritter, H., 1976. Monthly Not. Royal Astron. Soc., 175, 279.Google Scholar
Rucinski, S.M., 1974. Acta Astron., 24, 119.Google Scholar
Schatzman, E., 1962. Ann. Astrophys., 25, 18.Google Scholar
Semeniuk, I., and Paczynski, B., 1968. Acta Astron., 18, 33.Google Scholar
Shakura, N.I., 1972. Soviet Astronomy, 16, 756.Google Scholar
Shakura, N.I., and Sunyaev, R.A., 1973. Astron. Astrophys. 24, 337.Google Scholar
Shklovsky, I.S., 1967. Astrophys. J., 148, Ll.Google Scholar
Shu, F.H. Lubow, S.H., and Anderson, L., 1979. Astrophys. J., 229, 223.Google Scholar
Sikora, M., 1979. To be submitted to Nature.Google Scholar
Smak, J., 1967, Acta Astron., 26, 255.Google Scholar
Smak, J., 1976, Acta Astron., 26, 277.Google Scholar
Strom, K.M., and Strom, S.E., 1970. Astrophys. J., 162, 523.Google Scholar
Taam, R.E., Bodenheimer, P., and Ostriker, J.P., 1978. Astrophys. J., 222, 269.Google Scholar
Taylor, J.H., 1979. Highlights of Astronomy, Vol. 5, in press.Google Scholar
Thorne, K.S., and Aytkow, A., 1977. Astrophys. J., 212, 832.Google Scholar
Trimble, V., 1977. Monthly Not. Royal Astron. Soc., 178, 335.Google Scholar
Tutukov, A.V., and Yungelson, L.R. 1976. Astrofizika, 12, 521.Google Scholar
Tutukov, A., and Yungelson, L., 1979. IAU Symp. No. 83, p. 401, Conti, P.S. and de Loore, C.W.H. (eds).Google Scholar
van den Heuvel, E.P.J., and Heise, J., 1972. Nature Phys. Sci., 239, 67.Google Scholar
Webbink, R.F., 1975. Ph.D. Thesis, Univ. of Cambridge.Google Scholar
Webbink, R.F., 1976. Astrophys. J., 209, 829.Google Scholar
Webbink, R.F., 1979. IAU Colloquium No. 46, in press New Zealand.Google Scholar
Weber, S.V., 1979. Astrophys. J., 229, 327.Google Scholar
Wheeler, J.C., 1979. Astrophys. J., in press.Google Scholar
Ziolkowski, J., 1976. Astrophys. J., 204, 512.Google Scholar
Ziolkowski, J., 1977. Annals New York Acad. Sci., 302, 47.Google Scholar
Ziolkowski, J., 1979. IAU Symp. No. 83, p. 385, Conti, P.S. and de Loore, C.W.H. (eds).Google Scholar