The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing

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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.
4 pages, plain TEX, no figures

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/9993

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9504099
 http://arxiv.org/abs/astro-ph/9504099
 Acta Astron. 45 (1995) 345

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arXiv