The discrepancy between solar abundances and helioseismology

被引:108
|
作者
Antia, HM
Basu, S
机构
[1] Tata Inst Fundamental Res, Bombay 400005, Maharashtra, India
[2] Yale Univ, Dept Astron, New Haven, CT 06520 USA
来源
ASTROPHYSICAL JOURNAL | 2005年 / 620卷 / 02期
基金
美国国家科学基金会;
关键词
Sun : abundances; Sun : interior; Sun : oscillations;
D O I
10.1086/428652
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
There have been recent downward revisions of the solar photospheric abundances of oxygen and other heavy elements. These revised abundances along with OPAL opacities are not consistent with seismic constraints. In this work we show that the recently released Opacity Project opacity tables cannot resolve this discrepancy either. While the revision in opacities does not seem to resolve this conflict, an upward revision of neon abundance in the solar photosphere offers a possible solution to this problem.
引用
收藏
页码:L129 / L132
页数:4
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