Masses of the astrometric SB2 zeta Ori A
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🌌 astro-ph.SR
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massessystemzetaastrometriccomparedderiveddynamicensuring
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We report the first dynamic mass for an O-type supergiant, the interferometrically resolved SB2 system \zeta Ori A (O9.5Ib+B0/1). The separation of the system excludes any previous mass-transfer, ensuring that the derived masses can be compared to single star evolutionary tracks.
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Cited by 1 Pith paper
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