The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing
classification
🌌 astro-ph
keywords
starsdwarfsmassesmicrolensingnearbybrowndetermineddirect
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Microlensing of distant stars in the Milky Way by the nearby high proper motion stars offers a direct way to precisely measure the masses of single lower main sequence stars and brown dwarfs.
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