Abstract
Calculations show that the observed semi-detached binary systems of mass M 1 + M 2≈ 2.5 M ⊙ can be explained in terms of a mass exchange which starts after the central hydrogen in the original primary has been exhausted.
On leave of absence from the University of Oslo.
On leave of absence from the University of Göttingen.
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References
Giannone, P., Kohl, K. and Weigert, A.: 1968, Z. Astrophys. 68, 107.
Kippenhahn, R. and Weigert, A.: 1967, Z. Astrophys. 65, 251.
Paczynski, B.: 1966, 1967, Acta Astron. 16, 231; 17, 1.
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© 1969 D. Reidel Publishing Company, Dordrecht, Holland
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Refsdal, S., Weigert, A. (1969). Evolution Through Mass Exchange in Close Binary Systems of Total Mass 2.5 M ⊙ . In: Hack, M. (eds) Mass Loss from Stars. Astrophysics and Space Science Library, vol 13. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3405-0_32
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DOI: https://doi.org/10.1007/978-94-010-3405-0_32
Publisher Name: Springer, Dordrecht
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