Spectrophotometric properties of pre-main-sequence stars: The ε Chamaeleontis cluster

Monthly Notices of the Royal Astronomical Society

Volumn 389, Issue 3, 2008, Pages 1461-1469

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

^a Korea Astronomy and Space Science Institute (KASI)   (South Korea)

^b UNIVERSITY OF NEW SOUTH WALES   (Australia)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

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

Indexed keywords

STARS;

BROAD BANDS; LOWER RESOLUTION; MAIN SEQUENCE STARS; OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: Ε CHAMAELEONTIS; OPEN CLUSTERS AND ASSOCIATION: INDIVIDUAL; OPTICAL SPECTROSCOPY; PRE-MAIN SEQUENCES; PROPERTY; STARS: PRE-MAIN SEQUENCE; STARS:FUNDAMENTAL PARAMETERS;

COLOR;

EID: 51349123996     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13688.x     Document Type: Article

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