Lensing of Invisible Stars by Brown Dwarfs

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dc.creatorBouquet, Alain
dc.date1993-04-28
dc.date.accessioned2026-07-07T02:18:46Z
dc.date.available2026-07-07T02:18:46Z
dc.descriptionTo detect brown dwarfs in the dark galactic halo through gravitational lensing, experiments follow the luminosity of millions of stars to observe a few lensing events par year. The luminosity of a star too faint to be continuously followed can be temporarily increased above the detection limit by a lensing. The detection of these invisible stars would increase the number of events by a factor 2 to 7, and moreover their presence would confirm the lensing interpretation of events due to continuously monitored stars.
dc.description9p, LaTeX, PAR-LPTHE 93-02
dc.identifierhttps://arxiv.org/abs/astro-ph/9304025
dc.identifierhttp://arxiv.org/abs/astro-ph/9304025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9614
dc.subjectAstrophysics
dc.titleLensing of Invisible Stars by Brown Dwarfs
dc.typetext

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