Orbital parameters, masses and distance to β Centauri determined with the Sydney University Stellar Interferometer and high-resolution spectroscopy

Monthly Notices of the Royal Astronomical Society

Volumn 356, Issue 4, 2005, Pages 1362-1370

  Davis, J ^a   Mendez, A ^a   Seneta, E B ^a,d   Tango, W J ^a   Booth, A J ^a,e   O'Byrne, J W ^a   Thorvaldson, E D ^a,f   Ausseloos, M ^b   Aerts, C ^b,c   Uytterhoeven, K ^b  

^a UNIVERSITY OF SYDNEY   (Australia)

^b UNIVERSITY OF LEUVEN   (Belgium)

^c RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f CSIRO   (Australia)

Author keywords

Binaries: General; Stars: Distances; Stars: Fundamental parameters; Stars: Individual: centauri; Techniques: Interferometric; Techniques: Spectroscopic

Indexed keywords

INTERFEROMETERS; INTERFEROMETRY; SPECTROSCOPIC ANALYSIS; TELESCOPES;

BINARIES:GENERAL; INTERFEROMETER RESOLUTION; ORBITAL PARAMETERS; STAR: INDIVIDUAL: Β CENTAURI; STAR:DISTANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:FUNDAMENTAL PARAMETERS; STELLAR INTERFEROMETERS; TECHNIQUE: INTERFEROMETRIC; TECHNIQUES: SPECTROSCOPIC;

STARS;

EID: 13444310986     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08571.x     Document Type: Article

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