机构:
Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, ScotlandUniv St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
Vrielmann, S
[1
]
Horne, K
论文数: 0引用数: 0
h-index: 0
机构:
Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, ScotlandUniv St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
Horne, K
[1
]
Baptista, R
论文数: 0引用数: 0
h-index: 0
机构:
Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, ScotlandUniv St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
Baptista, R
[1
]
Hessman, FV
论文数: 0引用数: 0
h-index: 0
机构:
Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, ScotlandUniv St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
Hessman, FV
[1
]
机构:
[1] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
来源:
ACCRETION PHENOMENA AND RELATED OUTFLOWS: IAU COLLOQUIUM 163
|
1997年
/
121卷
关键词:
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present a new eclipse mapping technique, which is able to map distributions in physical parameters of accretion disks in ecliping cataclysmic variables.