Abstract
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.
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References
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© 1986 D. Reidel Publishing Company
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Hubrig, S. (1986). The age of ε UMa. In: Cowley, C.R., Dworetsky, M.M., Mégessier, C. (eds) Upper Main Sequence Stars with Anomalous Abundances. Astrophysics and Space Science Library, vol 125. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4714-6_55
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DOI: https://doi.org/10.1007/978-94-009-4714-6_55
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