机构:
Yale Univ, Dept Astron, New Haven, CT 06511 USAYale Univ, Dept Astron, New Haven, CT 06511 USA
Basu, S
[1
]
Christensen-Dalsgaard, J
论文数: 0引用数: 0
h-index: 0
机构:
Yale Univ, Dept Astron, New Haven, CT 06511 USAYale Univ, Dept Astron, New Haven, CT 06511 USA
Christensen-Dalsgaard, J
[1
]
Monteiro, MJPFG
论文数: 0引用数: 0
h-index: 0
机构:
Yale Univ, Dept Astron, New Haven, CT 06511 USAYale Univ, Dept Astron, New Haven, CT 06511 USA
Monteiro, MJPFG
[1
]
Thompson, MJ
论文数: 0引用数: 0
h-index: 0
机构:
Yale Univ, Dept Astron, New Haven, CT 06511 USAYale Univ, Dept Astron, New Haven, CT 06511 USA
Thompson, MJ
[1
]
机构:
[1] Yale Univ, Dept Astron, New Haven, CT 06511 USA
来源:
PROCEEDINGS OF THE SOHO 10/GONG 2000 WORKSHOP ON HELIO- AND ASTEROSEISMOLOGY AT THE DAWN OF THE MILLENNIUM
|
2001年
/
464卷
关键词:
asteroseismology;
solar-type stars;
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Seismology of solar-type stars other than the Sun becomes a realistic possibly with the upcoming MOST, COROT and MONS missions, and the ESA mission Eddington. We report on the results of experiments with artificial data from models of solar-type stars to assess further what we might learn about the internal structure of such stars.