The AB Doradus moving group

被引：164
作者：
Zuckerman, B
Song, I
Bessell, MS
机构：
[1] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[2] Australian Natl Univ, Res Sch Astron & Astrophys, Inst Adv Studies, Canberra, ACT 2611, Australia
[3] Univ Calif Los Angeles, Ctr Astrobiol, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
[4] AURA Gemini Observ, Hilo, HI 96720 USA
来源：
ASTROPHYSICAL JOURNAL | 2004年 / 613卷 / 01期
基金：
美国国家航空航天局;
关键词：
open clusters and associations : individual (AB Doradus moving group); stars : kinematics; stars : pre -main-sequence;
D O I：
10.1086/425036
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
From radio to X-ray wavelengths, AB Doradus has been an intensively studied star. We have identified similar to30 nearby star systems, each with one or more characteristics of youth, that are moving through space together with AB Dor. This diverse set of similar to50 million year old star systems is the comoving, youthful group closest to Earth. The group's nucleus is a clustering of a dozen stars similar to20 pc from Earth that includes AB Dor itself. The AB Dor moving group joins the previously known and somewhat younger and more distant Tucana/Horologium and TW Hydrae associations and the beta Pictoris moving group as excellent laboratories for investigations of forming planetary systems.
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页码：L65 / L68
页数：4
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