Rotation periods for stars of the TW Hydrae association: The evidence for two spatially and rotationally distinct pre-main-sequence populations

Monthly Notices of the Royal Astronomical Society

Volumn 357, Issue 4, 2005, Pages 1399-1406

  Lawson, Warrick A ^a   Crause, Lisa A ^b,c  

^a UNIVERSITY OF NEW SOUTH WALES   (Australia)

^b UNIVERSITY OF CAPE TOWN   (South Africa)

^c SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

Author keywords

Open clusters and associations: individual: TW Hydrae; Stars: activity; Stars: pre main sequence; Stars: rotation

Indexed keywords

STARS;

LATE-TYPE; OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: TW HYDRAE; OPEN CLUSTERS AND ASSOCIATION: INDIVIDUAL; PHOTOMETRICS; PRE-MAIN SEQUENCES; ROTATION PERIOD; STAR: ACTIVITY; STARS: PRE-MAIN SEQUENCE; STARS: ROTATION; TW HYDRAE;

PHOTOMETRY;

EID: 15244358913     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08793.x     Document Type: Article

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