Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances
Standard solar models (SSMs) constructed in accord with low metal abundances disagree with seismically inferred results. We constructed rotating solar models with low metal abundances that included enhanced settling and convection overshoot. In one of our rotating models, AGSSr2a, the convection ove...
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Veröffentlicht in: | The Astrophysical journal 2019-03, Vol.873 (1), p.18 |
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Sprache: | eng |
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