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

The bright southern binary star b Centauri (HR 5267) has been observed with the Sydney University Stellar Interferometer (SUSI) and spectroscopically with the European Southern Observatory Coude Auxiliary Telescope and Swiss Euler telescope at La Silla. The interferometric observations have confirme...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2005-02, Vol.356 (4), p.1362-1370
Hauptverfasser:	Davis, J, Mendez, A, Seneta, E B, Tango, W J, Booth, A J, O'Byrne, J W, Thorvaldson, E D, Ausseloos, M, Aerts, C, Uytterhoeven, K
Format:	Artikel
Sprache:	eng
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