The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing

Details The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing

1995-04-27

arxiv.org/abs/astro-ph/9504099v1

Acta Astron. 45 (1995) 345

Astronomy and Astrophysics

Astrophysics

4 pages, plain TEX, no figures

Scientific paper

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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