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
相关论文
共 50 条
  • [41] K nearest neighbors search for the trajectory of moving object
    Liu, XF
    Liu, YS
    Xiao, YY
    2005 INTERNATIONAL CONFERENCE ON WIRELESS COMMUNICATIONS, NETWORKING AND MOBILE COMPUTING PROCEEDINGS, VOLS 1 AND 2, 2005, : 1304 - 1307
  • [42] Nearest Neighbor Search on Moving Object Trajectories in SECONDO
    Gueting, Ralf Hartmut
    Braese, Angelika
    Behr, Thomas
    Xu, Jianqiu
    ADVANCES IN SPATIAL AND TEMPORAL DATABASES, PROCEEDINGS, 2009, 5644 : 427 - 431
  • [43] Nearest neighbor search for constrained moving objects trajectories
    College of Computer Science and Technology, Huazhong University of Science and Technology, Wuhan 430074, China
    Huazhong Ligong Daxue Xuebao, 2007, 2 (57-60):
  • [44] A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood
    Bell, Cameron P. M.
    Mamajek, Eric E.
    Naylor, Tim
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 454 (01) : 593 - 614
  • [45] Post T Tauri stars in the solar neighborhood: isolated or members of young associations and moving groups
    Montes, D.
    Lopez-Santiago, J.
    Martinez-Arnadiz, R. M.
    Guillout, P.
    Klutsch, A.
    Ferrero, R. Freire
    Frasca, A.
    Marilli, E.
    COOL STARS, STELLAR SYSTEMS AND THE SUN, 2009, 1094 : 943 - +
  • [46] The Elusive Majority of Young Moving Groups. I. Young Binaries and Lithium-rich Stars in the Solar Neighborhood
    Bowler, Brendan P.
    Hinkley, Sasha
    Ziegler, Carl
    Baranec, Christoph
    Gizis, John E.
    Law, Nicholas M.
    Liu, Michael C.
    Shah, Viyang S.
    Shkolnik, Evgenya L.
    Riaz, Basmah
    Riddle, Reed
    ASTROPHYSICAL JOURNAL, 2019, 877 (01):
  • [47] On the evolution of moving groups: an application to the Pleiades moving group
    Asiain, R
    Figueras, F
    Torra, J
    ASTRONOMY & ASTROPHYSICS, 1999, 350 (02): : 434 - 446
  • [48] Moving range k nearest neighbor queries with quality guarantee over uncertain moving objects
    Lee, Eun-Young
    Cho, Hyung-Ju
    Chung, Tae-Sun
    Ryu, Ki-Yeol
    INFORMATION SCIENCES, 2015, 325 : 324 - 341
  • [49] The Moving K Diversified Nearest Neighbor Query (Extended Abstract)
    Gu, Yu
    Liu, Guanli
    Qi, Jianzhong
    Xu, Hongfei
    Yu, Ge
    Zhang, Rui
    2017 IEEE 33RD INTERNATIONAL CONFERENCE ON DATA ENGINEERING (ICDE 2017), 2017, : 31 - 32
  • [50] Probabilistic k-Nearest Neighbor Monitoring of Moving Gaussians
    Patroumpas, Kostas
    Koutras, Christos
    SSDBM 2017: 29TH INTERNATIONAL CONFERENCE ON SCIENTIFIC AND STATISTICAL DATABASE MANAGEMENT, 2017,
12345