Zoom-In ON hIgh-mass Star forMation
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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Projects: Funded Project
Characterizing the smallest planet hosts
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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Breaking through outstanding problems in stellar evolution with ultra-precise space-based photometry (BreakStarS)
The last decade has witnessed a dramatic change in stellar astrophysics research as a result of the launch of space missions — such
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Revealing the Milky Way with Gaia (MW-GAIA)
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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