Beta Hydri (G2 IV): a revised age for the closest subgiant

被引:0
|
作者
Dravins, D
Lindegren, L
VandenBerg, DA
机构
[1] Lund Observ, S-22100 Lund, Sweden
[2] Univ Victoria, Dept Phys & Astron, Victoria, BC V8W 3P6, Canada
关键词
space astrometry; stars : evolution; stars : individual : beta Hyi; stars : late-type;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The secular evolution of solar-type atmospheres may be studied through comparisons of the current Sun with old solar-type stars of known age. Among the few such stars in the solar Galactic neighborhood, beta Hydri (G2 IV) stands out as a normal single star with an advanced age. Previous age determinations (similar or equal to 9.5 Gy) were based on the old ground-based parallax of 153 mas. The new Hipparcos value of 133.78+/-0.51 mas implies an absolute magnitude M-V = 3.43+/-0.01,0.3 mag brighter than previously believed. New evolutionary calculations produce best-fit models with ages around 6.7 Gy. Although the Hipparcos data thus lead to a significant reduction of its estimated age, beta Hyi remains an old star.
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收藏
页码:1077 / 1079
页数:3
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