Quantifying the contamination by old main-sequence stars in young moving groups: the case of the Local Association

Astronomy and Astrophysics

Volumn 499, Issue 1, 2009, Pages 129-135

  Lopez Santiago J ^a,b   Micela, G ^b   Montes, D ^a  

^a UNIVERSIDAD COMPLUTENSE DE MADRID   (Spain)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

Author keywords

Galaxy: solar neighborhood; Galaxy: stellar content; Stars: activity; Stars: coronae; Stars: kinematics

Indexed keywords

GALAXY: SOLAR NEIGHBORHOOD; GALAXY: STELLAR CONTENT; STARS: ACTIVITY; STARS: CORONAE; STARS: KINEMATICS;

CONTAMINATION; GALAXIES; KINEMATICS; LITHIUM; PHOTOMETRY; POPULATION STATISTICS;

STARS;

EID: 66349110890     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811590     Document Type: Article

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