The Gaia ultracool dwarf sample – II. Structure at the end of the main sequence

dc.creatorSmart R.L.
dc.creatorMarocco F.
dc.creatorSarro L.M.
dc.creatorBarrado D.
dc.creatorBeamín J.C.
dc.creatorCaballero J.A.
dc.creatorJones H.R.A.
dc.date.accessioned2020-09-02T22:28:02Z
dc.date.accessioned2022-11-08T20:28:21Z
dc.date.available2020-09-02T22:28:02Z
dc.date.available2022-11-08T20:28:21Z
dc.date.created2020-09-02T22:28:02Z
dc.date.issued2019
dc.identifier485, 3, 4423-4440
dc.identifier00358711
dc.identifierhttps://hdl.handle.net/20.500.12728/6172
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5146793
dc.languageen
dc.publisherOxford University Press
dc.subjectBinaries: visual
dc.subjectBrown dwarfs
dc.subjectHertzsprung–Russell and colour–magnitude diagrams
dc.subjectSolar neighbourhood
dc.subjectStars: late-type
dc.titleThe Gaia ultracool dwarf sample – II. Structure at the end of the main sequence
dc.typeArticle


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