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Young Pre-Main Sequence Stars: Accretion/Outflow, Planet Formation, and Contraction/Spin-Up on the Active Journey to a Main Sequence Life of Boredom

Published onMay 31, 2019
Young Pre-Main Sequence Stars: Accretion/Outflow, Planet Formation, and Contraction/Spin-Up on the Active Journey to a Main Sequence Life of Boredom
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Abstract

The field of star formation, young stellar objects, and pre-main sequence stars has benefited from the combined set of wide-field, multi-wavelength photometric surveys over the past two decades. What is currently lacking is a comparable effort in spectroscopy. This position paper makes the case that major spectroscopic investments are needed.

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