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- W2080499662 abstract "Observational data for Algol-type systems are discussed basing on available evolutionary tracks. It is shown that the observed properties of the massive binaries (with total mass greater than 5 m⊙) can be satisfactorily explained assuming that their contact components are burning hydrogen in the core (case A). On the contrary, the majority of contact components of the observed low-mass binaries are burning hydrogen in the shell. The observed distribution of such binaries as a function of different luminosity excesses seems to indicate that their origin is connected with systems in which the primary component reached the Roche lobe before exhaustion of hydrogen in its center. Some mass loss from the system as a whole seems to be necessary in this case." @default.
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- W2080499662 date "1969-01-01" @default.
- W2080499662 modified "2023-09-27" @default.
- W2080499662 title "Evolution of Close Binaries and Origin of Algol-Type Systems" @default.
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- W2080499662 doi "https://doi.org/10.1007/978-94-010-3405-0_29" @default.
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