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The Astrophysical Journal, 1(904), p. 82, 2020

DOI: 10.3847/1538-4357/abb5a6

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Characterizing the Evolved Stellar Population in the Galactic Foreground. I. Bolometric Magnitudes, Spatial Distribution and Period–Luminosity Relations

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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