The Chemical Composition of the Extreme Halo Stars HE 0107-5420 and HE 1327-2326 Inferred from Three-dimensional Hydrodynamical Model Atmospheres

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dc.contributor.authorCollet, Remo
dc.contributor.authorAsplund, Martin
dc.contributor.authorTrampedach, Regner
dc.date.accessioned2015-12-07T22:53:07Z
dc.date.available2015-12-07T22:53:07Z
dc.date.issued2006
dc.date.updated2015-12-07T12:36:58Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/27718
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.titleThe Chemical Composition of the Extreme Halo Stars HE 0107-5420 and HE 1327-2326 Inferred from Three-dimensional Hydrodynamical Model Atmospheres
dc.typeJournal article
local.bibliographicCitation.lastpageL124
local.bibliographicCitation.startpageL121
local.contributor.affiliationCollet, Remo, Uppsala University
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationTrampedach, Regner, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidAsplund, Martin, u4042723
local.contributor.authoruidTrampedach, Regner, u4089367
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4114753xPUB53
local.identifier.citationvolume644
local.type.statusPublished Version

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