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

The bright southern binary star beta Centauri (HR 5267) has been observed with the Sydney University Stellar Interferometer (SUSI) and spectroscopically with the ESO CAT and Swiss Euler telescopes at La Silla. The interferometric observations have confirmed the binary nature of the primary component...

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Veröffentlicht in:	arXiv.org 2004-11
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
Schlagworte:	Binary stars Binary system European Southern Observatory Inclination Interferometry Orbits Parameters Space telescopes Spectroscopic telescopes
Online-Zugang:	Volltext
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