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Spectroscopic distances of nearby ultracool dwarfs

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Phan-Bao, N; Bessell, Michael

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We present updated results of spectroscopic follow-up observations of a sample of 45 M dwarf candidates identified by Phan-Bao et al. (2003, A&A, 401, 959) based on the DENIS photometry and proper motion measurements. Forty one of these are nearby late-M

dc.contributor.authorPhan-Bao, N
dc.contributor.authorBessell, Michael
dc.date.accessioned2015-12-13T22:52:21Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/81524
dc.description.abstractWe present updated results of spectroscopic follow-up observations of a sample of 45 M dwarf candidates identified by Phan-Bao et al. (2003, A&A, 401, 959) based on the DENIS photometry and proper motion measurements. Forty one of these are nearby late-M
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Dust; Photometry; Spectroscopic analysis; Spectrum analysis; Motion measurements; Spectroscopic distances; Stars: low-mass, brown dwarfs; Ultracool dwarfs; Astrophysics Stars: low-mass, brown dwarfs
dc.titleSpectroscopic distances of nearby ultracool dwarfs
dc.typeJournal article
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.citationvolume446
dc.date.issued2006
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub9805
local.type.statusPublished Version
local.contributor.affiliationPhan-Bao, N, Academia Sinica
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.startpage515
local.bibliographicCitation.lastpage523
local.identifier.doi10.1051/0004-6361:20054064
dc.date.updated2015-12-11T10:50:35Z
local.identifier.scopusID2-s2.0-31544475414
CollectionsANU Research Publications

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