Abstract
The evolution of three close binary systems of total mass 20.4M ⊙ in and after the phase of mode Br mass-transfer in caseA of mass exchange is investigated. In every case a secondary component evolves to interfere with the progress of primary's evolution and the system overflows the outer critical surface before the primary completes its nuclear-burning evolution. This strongly indicates the importance of simultaneous calculation of both components. A summary of evolution of the systems considered in this series of papers up to the stage ofL 2-overflow is given. The observational aspects of the numerical models are also discussed.
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Andersen, J., Clausen, J. V., Giménez, A., and Nordström, B.: 1983,Astron. Astrophys. 118, 17.
Chambliss, C. R. and Leung, K.-C.: 1979,Astrophys. J. 228, 828.
De Grève, J. P.: 1980,Space Sci. Rev. 26, 113.
Giuricin, G. and Mardirossian, F.: 1981,Astrophys. J. Suppl. 46, 1.
Hall, D. S.: 1975,Acta Astron. 25, 1.
Hilditch, R. W.: 1984,Monthly Notices Roy. Astron. Soc. 211, 943.
Horn, J.: 1971,Bull. Astron. Inst. Czech. 22, 37.
Jiang, Z., Leung, K.-C., and Shen, L.: 1983,Astron. J. 88, 1679.
Kraitcheva, Z. T.: 1978,Nauch. Inform. 41, 37.
Leung, K.-C.: 1977, in E. A. Müller and A. Jappel (eds.),Transactions IAU XVIB, 283.
Massey, P.: 1982, in C. W. H. de Loore and A. J. Willis (eds.), ‘Wolf-Rayet Stars: Observations, Physics, Evolution’,IAU Symp. 99, 251.
Mezzetti, M., Giuricin, G., and Mardirossian, F.: 1980,Astron. Astrophys. 83, 217.
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.: 1987,Astrophys. Space Sci. 134, 161 (Paper II).
Plavec, M.: 1973, in A. H. Batten (ed.), ‘Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems’,IAU Symp. 51, 216.
Popper, D. M.: 1980,Ann. Rev. Astron. Astrophys. 18, 115.
Sybesma, C. H. B.: 1985,Astron. Astrophys. 142, 171.
Sybesma, C. H. B.: 1986,Astron. Astrophys. 159, 108.
Tutukov, A., Yungelson, J., and Klayman, A.: 1973,Nauch. Inform. 27, 3.
Ulrich, R. K.: 1972,Astrophys. J. 172, 165.
Vanbeveren, D. and de Loore, C.: 1980,Astron. Astrophys. 86, 21.
Webbink, R. F.: 1976,Astrophys. J. Suppl. 32, 583.
Wilson, R. E. and Rafert, J. B.: 1981,Astrophys. Space Sci. 76, 23.
Ziółkowski, J.: 1970,Acta Astron. 20, 213.
Ziółkowski, J.: 1976, in P. Eggleton, S. Mitton, and J. Whelan (eds.), ‘Structure and Evolution of Close Binary Systems’,IAU Symp. 73, 321.
Ziółkowski, J.: 1979, in P. S. Conti and C. W. H. de Loore (eds.), ‘Mass Loss and Evolution of O-Type Stars’,IAU Symp. 83, 385.
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Nakamura, M., Nakamura, Y. Case a evolution of massive close binary systems. Astrophys Space Sci 134, 219–234 (1987). https://doi.org/10.1007/BF01094934
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DOI: https://doi.org/10.1007/BF01094934