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Abstract

We have revisited the calibration of the visual binary system ζ Herculis with the goal to give the seismological properties of the G0 IV sub-giant ζ Her A. The sum of masses and the mass fraction are derived from the most recent astrometric data mostly based on the hipparco

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EDP Sciences OAI-PMH repository (1.2.0)

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Last time updated on 10/04/2020

This paper was published in EDP Sciences OAI-PMH repository (1.2.0).

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