The theory of high-mass star formation predicts specific features, namely, the formation of near-equal binary systems, radiative Rayleigh-Taylor instabilities, and bloated photospheres. The
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The determination of accurate and precise stellar parameters and chemical abundances of M dwarfs is of prime importance to the study of Galactic
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MW-GAIA will provide European leadership in understanding the Galaxy, its stars and planets, enhance the potential of the community in its scientific exploitation
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