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The Age of ε Uma

Published online by Cambridge University Press:  12 April 2016

S. Hubrig*
Affiliation:
Zentralinstitut für Astrophysik der AdW der DDRPotsdam, DDR

Abstract

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A critical rediscussion of the luminosity confirms that ε UMa is brighter than expected for a star on the main sequence, in our determination by 0m.6.

Type
Section III - Magnetic CP Stars
Copyright
Copyright © Reidel 1986

References

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