Chemical gradients in the Milky Way from the RAVE data: II. Giant stars

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dc.contributor.authorFreeman, Kenneth
dc.contributor.authorBoeche, C
dc.contributor.authorSiebert, A
dc.contributor.authorPiffl, T.
dc.contributor.authorJust, A.
dc.contributor.authorSteinmetz, Matthias
dc.contributor.authorGrebel, E.
dc.contributor.authorSharma, S
dc.contributor.authorKordopatis, G
dc.contributor.authorGilmore, Gerard
dc.contributor.authorChiappini, C
dc.date.accessioned2015-12-13T22:31:00Z
dc.date.issued2014
dc.date.updated2015-12-11T08:58:26Z
dc.description.abstractAims. We provide new constraints on the chemo-dynamical models of the Milky Way by measuring the radial and vertical chemical gradients for the elements Mg, Al, Si, Ti, and Fe in the Galactic disc and the gradient variations as a function of the distance
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/75102
dc.publisherSpringer
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstronomy and Astrophysics
dc.titleChemical gradients in the Milky Way from the RAVE data: II. Giant stars
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.contributor.affiliationFreeman, Kenneth, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBoeche, C, Zentrum fur Astronomie der Universitat Heidelberg
local.contributor.affiliationSiebert, A, Université de Strasbourg
local.contributor.affiliationPiffl, T., Rudolf Peierls Centre for Theoretical Physics
local.contributor.affiliationJust, A., Zentrum für Astronomie der Universität Heidelberg
local.contributor.affiliationSteinmetz, Matthias, Astrophysical Institute Potsdam
local.contributor.affiliationGrebel, E., Universitat Heidelberg
local.contributor.affiliationSharma, S, University of Sydney
local.contributor.affiliationKordopatis, G, University of Cambridge
local.contributor.affiliationGilmore, Gerard, University of Cambridge
local.contributor.affiliationChiappini, C, Leibniz-Institut fur Astrophysik Potsdam
local.contributor.authoruidFreeman, Kenneth, u7000399
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationU3488905xPUB4467
local.identifier.citationvolume568
local.identifier.doi10.1051/0004-6361/201423974
local.identifier.scopusID2-s2.0-84906255557
local.type.statusPublished Version

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