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Establishing an Empirical Substellar Sequence to Planetary Masses

Published onMay 31, 2019
Establishing an Empirical Substellar Sequence to Planetary Masses
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Abstract

Mass is the most fundamental parameter governing the life-history of all gaseous objects from stars to brown dwarfs and giant planets. Extending measurements of mass to the regime of directly imaged gas-giants, and spectroscopically characterizing this mass sample, will require the leap in angular resolution and sensitivity offered by the ELTs.

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