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- W1978406186 abstract "The structural and evolutionary conditions which allow high mass stars |$(M,lt,4,{M}_{odot})$| to become Cepheid variables are examined. The important internal parameters for determining the location of stars in H–R diagram are isolated from computed sequences of static models. It is demonstrated that the existence of a (reasonably long lived) Cepheid phase depends largely on the composition profil near the shell source. The interplay of the various processes which take place during actual evolution is concisely expressed in a semi-empirical relation between effective temperature and core mass (or helium content in the core) for the static situation. A qualitative interpretation of the computed results is offered." @default.
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- W1978406186 date "1972-02-01" @default.
- W1978406186 modified "2023-09-27" @default.
- W1978406186 title "Evolutionary Aspects of the Cepheid Stage" @default.
- W1978406186 doi "https://doi.org/10.1093/mnras/156.2.129" @default.
- W1978406186 hasPublicationYear "1972" @default.
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