Updating standard solar models

被引：64

作者：

Ciacio, F

Degl'Innocenti, S

Ricci, B

机构：

[1] UNIV FERRARA, DIPARTMENTO FIS, I-44100 FERRARA, ITALY

[2] MAX PLANCK INST ASTROPHYS, D-85740 GARCHING, GERMANY

[3] IST NAZL FIS NUCL, SEZIONE FERRARA, I-44100 FERRARA, ITALY

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1997年 / 123卷 / 03期

关键词：

the Sun; evolution; general; particle emission;

D O I：

10.1051/aas:1997168

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present an updated version of our standard solar model (SSM) where helium and heavy elements diffusion is included and the improved OPAL equation of state (Rogers 1994; Rogers et al. 1996) is used. In such a way the EOS is consistent with the adopted opacity tables, from the same Livermore group, an occurrence which should further enhance the reliability of the model. The results for the physical characteristics and the neutrino production of our SSM are discussed and compared with previous works on the matter.

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页码：449 / 454

页数：6

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