Abstract
We present in this paper the evolutionary characteristics of the systems belonging to two evolution types, designated as 1C2COf and 1Nc2COf, among seven evolution types which were studied in the preceding paper of this series. These two types are most complicated and interesting in the evolutionary behaviour, which consists of repeated detached, semi-detached, and contact phases. We discuss observational aspects of the results. Evolutionary behaviour of the systems are also discussed, compared with the thermal relaxation oscillation model.
Similar content being viewed by others
References
Andersen, J., Clausen, J. V., Giménez, A., and Nordström, B.: 1983,Astron. Astrophys. 128 17.
Andersen, J., Nordström, B., and Wilson, R. E.: 1980,Astron. Astrophys. 82, 225.
Batten, A. H., Fletcher, J. M., and Mann, P. J.: 1978,Publ. Dominion Astrophys. Obs. 15, 121.
Bondarenko, I. I. and Istomin, L. F.: 1980,Peremenye Zvezdy 21, 445.
Chambliss, C. R. and Leung, K.-C.: 1979,Astrophys. J. 228, 828.
De Greve, J. P.: 1986,Space Sci. Rev. 43, 139.
Drechsel, H., Rahe, J., Wargau, W., and Wolf, B.: 1982,Astron. Astrophys. 110, 246.
Eaton, J. A.: 1978,Acta Astron. 28, 63.
Flannery, B. P.: 1976,Astrophys. J. 205, 217.
Giuricin, G. and Mardirossian, F.: 1981,Astrophys. J. Suppl. 46, 1.
Hilditch, R. W.: 1984,Monthly Notices Roy. Astron. Soc. 211, 943.
Kippenhahn, R. and Thomas, H.-C.: 1980, in J. Ehlers, J. J. Perry, and M. Walker (eds.),9th Texas Symp. on Relativistic Astrophys. 9, 579.
Leung, K.-C. and Schneider, D. P.: 1977,Astrophys. J. 211, 844.
Leung, K.-C., Sistero, R. F., Zhai, D.-S., Grieco, A., and Candellero, B.: 1984,Astron. J. 89, 872.
Li, Y.-F. and Leung, K.-C.: 1985,Astrophys. J. 298, 345.
Lucy, L. B.: 1976,Astrophys. J. 205, 208.
Lucy, L. B. and Wilson, R. E.: 1979,Astrophys. J. 231, 502.
Mammano, A., Margoni, R., and Stagni, R.: 1977,Astron. Astrophys. 59, 9.
Nakamura, M. and Nakamura, Y.: 1982,Astrophys. Space Sci. 83, 163.
Nakamura, M. and Nakamura, Y.: 1984,Astrophys. Space Sci. 104, 367 (Paper I).
Nakamura, M. and Nakamura, Y.: 1985,Publ. Astron. Soc. Japan 37, 545.
Paczyński, B.: 1971,Ann. Rev. Astron. Astrophys 9, 183.
Plavec, M., Kříž, S., and Horn, J.: 1969,Bull. Astron. Inst. Czech. 20, 41.
Popper, D. M.: 1980,Ann. Rev. Astron. Astrophys. 18, 115.
Popper, D. M.: 1982,Astrophys. J. 262, 641.
Robertson, J. A. and Eggleton, P. P.: 1977,Monthly Notices Roy. Astron. Soc. 179, 359.
Schneider, D. P., Darland, J. J., and Leung, K.-C.: 1979,Astron. J. 84, 236.
Sezer, C., Güdür, N., Gülmen, Ö, and Şengonca, H.: 1983,Astron. Astrophys. Suppl. 53, 363.
Thomas, H.-C.: 1977,Ann. Rev. Astron. Astrophys. 15, 127.
Vanbeveren, D. and de Loore, C.: 1980,Astron. Astrophys. 86, 21.
Van der Veen, W. E. C. J.: 1985,Astron. Astrophys. 145, 380.
Webbink, R. F.: 1980, in M. J. Plavec, D. M. Popper, and R. K. Ulrich (eds.), ‘Close Binary Stars: Observations and Interpretation’,IAU Symp. 88, 127.
Wilson, R. E. and Leung, K.-C.: 1977.Astron. Astrophys. 61, 137.
Wilson, R. E. and Starr, T. C.: 1976,Monthly Notices Roy. Astron. Soc. 176, 625.
Yungelson, L. R. and Massevich, A. G.: 1983,Astrophys. Space Phys. Rev. 2, 29.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Nakamura, M., Nakamura, Y. Case a evolution of massive close binary systems. Astrophys Space Sci 134, 161–176 (1987). https://doi.org/10.1007/BF00636463
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00636463