机构:
Brigham Young Univ, Dept Phys & Astron, Provo, UT 84602 USABrigham Young Univ, Dept Phys & Astron, Provo, UT 84602 USA
McNamara, D. H.
[1
]
机构:
[1] Brigham Young Univ, Dept Phys & Astron, Provo, UT 84602 USA
来源:
STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION
|
2009年
/
1170卷
关键词:
delta Scuti stars: pulsating blue stragglers;
SX Phe stars;
BLUE STRAGGLERS;
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We describe the ages of delta Scuti stars as a function of the fundamental period of pulsation. We show that the metal-poor variables (pulsating blue stragglers or SX Phe stars) should be restricted to short periods as observed. The metal-strong variables on the other hand, should show a much greater range of periods, but LogP >= -1.3 days.