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- W2949416750 abstract "We investigate the effects of a modification of the $^{14}$N(p,{gamma})$^{15}$O reaction rate, as suggested by recent evaluations, on the formation and extension of the blue loops encountered during the evolution of the stars in the mass range 5M$_{odot}$ to 12M$_{odot}$. We show that the blue loops of stars in the mass range 5M$_{odot}$ to 8M$_{odot}$, that is the range of super ABG stars, are severely affected by a modification of the important $^{14}$N(p,{gamma})$^{15}$O reaction rate. We also show that the blue loops can be restored if envelope overshooting is included, which is necessary to explain the observations of the Cepheid stars." @default.
- W2949416750 created "2019-06-27" @default.
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- W2949416750 date "2014-10-07" @default.
- W2949416750 modified "2023-09-27" @default.
- W2949416750 title "Sensitivity of the Blue Loops of Intermediate-Mass Stars to Nuclear Reactions" @default.
- W2949416750 hasPublicationYear "2014" @default.
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