Title of article
Beryllium depletion in the solar atmosphere
Author/Authors
Xiong Da-run and Deng Li-cai، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2003
Pages
3
From page
1
To page
3
Abstract
Using a non-local convection theory for chemically inhomogeneous stars, the beryllium depletion of the Sun is calculated. The results show that Be is slightly depleted (∼5%) in the evolutionary model for the Sun.
Keywords
SUN , abundance-stars , abundances-convection
Journal title
Chinese Astronomy and Astrophysics
Serial Year
2003
Journal title
Chinese Astronomy and Astrophysics
Record number
2263277
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