A KINEMATIC STUDY OF THE LUPUS STAR-FORMING REGION

被引：0
|
作者：
Galli, P. A. B. [1 ]
Bertout, C. [2 ]
Teixeira, R. [1 ]
Ducourant, C. [3 ]
机构：
[1] Univ Sao Paulo, IAG, Inst Astron Geofis & Ciencias Atmosfer, Rua Matao 1226,Cidade Univ, BR-05508900 Sao Paulo, Brazil
[2] Inst Astrophys Paris, F-75014 Paris, France
[3] CNRS UMR 5804, Observ Aquitain Sci Univers, Floirac, France
来源：
XIV LATIN AMERICAN REGIONAL IAU MEETING | 2014年 / 44卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper, we study the southern star forming region located in Lupus that constitutes one of the richest associations of T Tauri stars. Based on the convergent point (CP) method combined with a k-NN analysis we identify 109 pre-main sequence stars in this region that define the Lupus association of co-moving stars, and derive individual distances for all group members.
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页码：28 / 28
页数：1
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