The nearest young moving groups

被引：145
|
作者：
Lopez-Santiago, J.
Montes, D.
Crespo-Chacon, I.
Fernandez-Figueroa, M. J.
机构：
[1] Osserv Astron Palermo, INAF, I-90134 Palermo, Italy
[2] Univ Complutense Madrid, Fac Ciencias Fis, Dept Astrofis & Ciencias Atmosfera, E-28040 Madrid, Spain
来源：
ASTROPHYSICAL JOURNAL | 2006年 / 643卷 / 02期
关键词：
open clusters and associations : general; planetary systems; stars : abundances; stars : activity; stars : kinematics;
D O I：
10.1086/503183
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The latest results in the research of forming planetary systems have led several authors to compile a sample of candidates for searching for planets in the vicinity of the Sun. Young stellar associations are indeed excellent laboratories for this study, but some of them are not close enough to allow the detection of planets through adaptive optics techniques. However, the existence of very close young moving groups can solve this problem. Here we have compiled the members of the nearest young moving groups, as well as a list of new candidates from our catalog of late-type stars that are possible members of young stellar kinematic groups, studying their membership through spectroscopic and photometric criteria.
引用
收藏
页码：1160 / 1165
页数：6
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