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- W3024794304 abstract "We present a grid of evolutionary computations of stellar structures with an original amount of heavy elements Z = 10 −10 and for an original He abundance Y = 0.23. The range of stellar masses 0.7 ≤ M ≤ 15 M ○. has been investigated, following the evolution from the initial ZAMS structures till the He flash or, for larger masses, up to the final cooling of the C-O degenerate cores or up to the C ignition. Parallel computations are presented for Z = 10 −6 and Z = 10 −4 , allowing the investigation of the evolutionary behavior of stellar structures when lowering the metallicity from a normal Population II composition down to the expected cosmological abundance of heavy elements" @default.
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- W3024794304 date "1993-01-01" @default.
- W3024794304 modified "2023-09-26" @default.
- W3024794304 title "An evolutionary scenario for primeval stellar populations" @default.
- W3024794304 hasPublicationYear "1993" @default.
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