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CaseA evolution of massive close binary systems

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Abstract

The caseA evolution of close binary systems with total mass of 20.4M ⊙ is investigated by following the evolution of both components simultaneously. The evolution is followed up to the stage at which a system overflows the outer critical surface or evolves into the phase of modeBr mass-transfer. It is found that the evolution of the systems can be classified into six types. The ranges of initial parameters which lead systems to each type of evolution are shown on the initial-parameter plane. The evolutionary features of each evolution type are described in detail.

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References

  • Giuricin, G. and Mardirossian, F.: 1981,Astrophys. J. Suppl. 46, 1.

    Google Scholar 

  • Giuricin, G., Mardirossian, F., and Mezzetti, M.: 1983,Astrophys. J. Suppl. 52, 35.

    Google Scholar 

  • Kippenhahn, R. and Meyer-Hofmeister, E.: 1977,Astron. Astrophys. 54, 539.

    Google Scholar 

  • Leung, K.-C.: 1977, in E. A. Muller and A. Jappel (eds.),Transactions IAU XVIB, 283.

    Google Scholar 

  • Mezzetti, M., Giuricin, G., and Mardirossian, F.: 1980,Astron. Astrophys. 83, 217.

    Google Scholar 

  • Nakamura, M. and Nakamura, Y.: 1982,Astrophys. Space Sci. 83, 163.

    Google Scholar 

  • Neo, S., Miyaji, S., Nomoto, K., and Sugimoto, D.: 1977,Publ. Astron. Soc. Japan 29, 249.

    Google Scholar 

  • Packet, W. and De Grève, J. P.: 1979,Astron. Astrophys. 75, 255.

    Google Scholar 

  • Plavec, M., Kříž, S., and Horn, J.: 1969,Bull. Astron. Inst. Czech. 20, 41.

    Google Scholar 

  • Tutukov, A. V., Yungelson, L. R., and Klayman, A. J.: 1973,Nauch. Inform. 27, 3.

    Google Scholar 

  • Webbink, R. F.: 1976,Astrophys. J. Suppl. 32, 583.

    Google Scholar 

  • Wilson, R. E. and Rafert, J. B.: 1981,Astrophys. Space Sci. 76, 23.

    Google Scholar 

  • Żiółkowski, J.: 1969,Astrophys. Space Sci. 3, 14.

    Google Scholar 

  • Żiółkowski, J.: 1970,Acta Astron. 20, 213.

    Google Scholar 

  • Żiółkowski, 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.

    Google Scholar 

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Authors and Affiliations

  1. Astronomical Institute, Tohoku University, Sendai, Miyagi, Japan

    Masaomi Nakamura

  2. Komaba High School, Ohashi, Meguro-ku, Tokyo, Japan

    Yasuhisa Nakamura

Authors
  1. Masaomi Nakamura
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  2. Yasuhisa Nakamura
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Nakamura, M., Nakamura, Y. CaseA evolution of massive close binary systems. Astrophys Space Sci 104, 367–387 (1984). https://doi.org/10.1007/BF00650310

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  • DOI: https://doi.org/10.1007/BF00650310

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