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- W98307205 abstract "Evolutionary tracks are presented for 2, 3, 10, 12, and 30 M/sup sub solar / stars having X = 0.7 and Z = 0.001. Both the main sequence and the Hayashi limit are bluer than for metal-rich stars, and the main-sequence models have higher luminosities, central temperatures and densities, and smaller radii. The higher luminosity shortens the time scales of the evolution for a given mass. Helium burning occurs close to the main sequence for the 10, 12, and 30 M/sub sub solar / models, rather than in the red giant phase. These differences can be understood qualitatively. The main sequence convective cores, and thus the helium cores formed, are larger than for corresponding higher Z model. Metal- poor stars are therefore capable of contributing a larger amount of helium to the galaxy than metal-rich stars. (auth)" @default.
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- W98307205 date "1973-05-01" @default.
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- W98307205 title "Evolution of massive population II stars" @default.
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