The nearby M-dwarf system Gliese 866 revisited

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dc.creatorWoitas, Jens
dc.creatorLeinert, Christoph
dc.creatorJahreiß, Hartmut
dc.creatorHenry, Todd
dc.creatorFranz, Otto
dc.creatorWasserman, Larry
dc.date1999-10-22
dc.date.accessioned2026-07-07T02:34:00Z
dc.date.available2026-07-07T02:34:00Z
dc.descriptionWe present an improved orbit determination for the visual pair in the M-dwarf triple system Gliese 866 that is based on new speckle-interferometric and HST observations. The system mass is M = 0.34 +- 0.03 solar masses. The masses of the components derived using the mass-luminosity relation are consistent with this mass sum. All three components of Gliese 866 seem to have masses not far from the hydrogen burning mass limit.
dc.description4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9910411
dc.identifierhttp://arxiv.org/abs/astro-ph/9910411
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15071
dc.subjectAstrophysics
dc.titleThe nearby M-dwarf system Gliese 866 revisited
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