KINEMATICS AND VELOCITY ELLIPSOID OF THE SOLAR NEIGHBORHOOD WHITE DWARFS

被引:0
|
作者
Elsanhoury, W. H. [1 ,2 ]
Nouh, M. I. [1 ,3 ]
Abdel-Rahman, H. I. [1 ,4 ]
机构
[1] Natl Res Inst Astron & Geophys, Dept Astron, Cairo 11421, Egypt
[2] Northern Border Univ, Fac Sci & Arts, Dept Phys, Rafha Branch, Ar Ar, Saudi Arabia
[3] Northern Border Univ, Coll Sci, Dept Phys, Ar Ar, Saudi Arabia
[4] Shaqraa Univ, Fac Sci, Dept Math, Shaqraa, Saudi Arabia
关键词
solar neighborhood; stars: kinematics and dynamics; stars: white dwarfs; COOLING SEQUENCE; SUN KINEMATICS; HIPPARCOS DATA; M4;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
To determine the velocity ellipsoid of the solar neighborhood white dwarfs, we use the space velocity components of stars. Two samples of white dwarfs are used, the 20 pc and 25 pc samples. Beside the two main samples, the solar velocity and velocity dispersions are calculated for four subsamples, namely BA, non - DA, hot and cool white dwarfs. A comparison between the results of the 20 pc sample and those of the 25 pc sample gives good agreement, while the comparison between the other subsamples gives poor agreement. The dependence of the velocity dispersions and solar velocity on the chemical composition and effective temperatures is discussed.
引用
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页码:197 / 206
页数:10
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