The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing

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dc.creatorPaczynski, B.
dc.date1995-04-27
dc.date.accessioned2026-07-07T02:19:45Z
dc.date.available2026-07-07T02:19:45Z
dc.descriptionMicrolensing 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.
dc.description4 pages, plain TEX, no figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9504099
dc.identifierhttp://arxiv.org/abs/astro-ph/9504099
dc.identifierActa Astron. 45 (1995) 345
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9993
dc.subjectAstrophysics
dc.titleThe Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing
dc.typetext

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