Estimation of Stellar Metal Abundance. II. A Recalibration of the Ca II K Technique, and the Autocorrelation Function Method

dc.contributor.authorBeers, Timothy C
dc.contributor.authorRossi, Silvia
dc.contributor.authorNorris, John
dc.contributor.authorRyan, Sean G
dc.contributor.authorShelfer, T
dc.date.accessioned2015-12-13T23:40:24Z
dc.date.available2015-12-13T23:40:24Z
dc.date.issued1999
dc.date.updated2015-12-12T09:29:01Z
dc.description.abstractWe have recalibrated a method for the estimation of stellar metal abundance, parameterized as [Fe/H], based on medium-resolution (1-2 Å) optical spectra (the majority of which cover the wavelength range 3700-4500 Å). The equivalent width of the Ca II K
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/94449
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Galaxy: abundances; Galaxy: halo; Stars: population II
dc.titleEstimation of Stellar Metal Abundance. II. A Recalibration of the Ca II K Technique, and the Autocorrelation Function Method
dc.typeJournal article
local.bibliographicCitation.lastpage1009
local.bibliographicCitation.startpage981
local.contributor.affiliationBeers, Timothy C, Michigan State University
local.contributor.affiliationRossi, Silvia, Universidade de Sao Paulo
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRyan, Sean G, Open University
local.contributor.affiliationShelfer, T, Michigan State University
local.contributor.authoremailu7401084@anu.edu.au
local.contributor.authoruidNorris, John, u7401084
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub24044
local.identifier.citationvolume117
local.identifier.scopusID2-s2.0-0000815530
local.identifier.uidSubmittedByMigrated
local.type.statusPublished Version

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