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A Peculiar Effect of Core Overshooting on the Internal Structure of Low-Mass Stars

Published online by Cambridge University Press:  12 April 2016

Nami Mowlavi
Nami Mowlavi*
Affiliation:
Institut d’Astronomie et d’Astrophysiqué;, Université Libre de Bruxelles, C.P. 165; Av. F.-D. Roosevelt, 50, 1050 Bruxelles, BELGIUM

Abstract

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With the aid of detailed stellar model computations, we analyse the consequences of applying a mild overshooting to 1.0 M⊙ to 1.2 M⊙ stars with solar metallicity. It is shown that solar models with a small convective core can be constructed, resulting in a decrease in the 8B neutrino flux that can amount to 30% relative to the value obtained in models without convective core.

Type
V. The changing interior
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 454 - 456
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Anders, E. and Grevesse, N. 1989, Geochem. Cosmochem. Acta, 53,197 CrossRefGoogle Scholar
Forestini, M. 1991, Ph.D. Thesis (Université Libre de Bruxelles)Google Scholar
Maeder, A. and Meynet, G. 1989, Astr. Ap., 210,155 Google Scholar
Mowlavi, N. and Forestini, M. 1992, in preparationGoogle Scholar
Provost, J., Berthomieu, G., Gavryuseva, E. and Gavryusev, V. 1990, Solar Physics, 128, 111 Google Scholar
Schaller, G., Schaerer, D., Meynet, G. and Maeder, A. 1992, preprintGoogle Scholar
Sienkiewicz, R., Bahcall, J.N. and Paczyński, B. 1990, Ap. J., 349, 641 Google Scholar
Zahn, J.-P. 1991, Astr. Ap., 252, 179 Google Scholar