The spectroscopic characteristics of intermediate-aged pre-main-sequence stars: The η Chamaeleontis cluster

Monthly Notices of the Royal Astronomical Society

Volumn 355, Issue 2, 2004, Pages 363-373

  Lyo, A Ran ^a,b   Lawson, Warrick A ^a   Bessell, M S ^c  

^a UNIVERSITY OF NEW SOUTH WALES   (Australia)

^b INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

Open clusters and associations: individual: Chamaeleontis; Stars: fundamental parameters; Stars: pre main sequence

Indexed keywords

ASTROPHYSICS; STARS;

MAIN SEQUENCE STARS; METALLICITIES; NARROW BANDS; OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: Η CHAMAELEONTIS; OPEN CLUSTERS AND ASSOCIATION: INDIVIDUAL; PRE-MAIN SEQUENCES; SPECTROSCOPIC CHARACTERISTICS; STARS: BE; STARS: PRE-MAIN SEQUENCE; STARS:FUNDAMENTAL PARAMETERS;

COLOR;

EID: 10444263815     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08318.x     Document Type: Article

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