New light on stellar abundance analyses: Departures from LTE and homogeneity.

dc.contributor.authorAsplund, Martin
dc.date.accessioned2015-12-13T22:48:38Z
dc.date.issued2005
dc.date.updated2015-12-11T10:29:40Z
dc.description.abstractThe information on the chemical compositions of stars encoded in their spectra plays a central role in contemporary astrophysics. Stellar element abundances are, however, not observed: to decipher the spectral fingerprints in terms of abundances requires
dc.identifier.issn0066-4146
dc.identifier.urihttp://hdl.handle.net/1885/80168
dc.publisherAnnual Reviews Inc
dc.sourceAnnual Review of Astronomy and Astrophysics
dc.subjectKeywords: Convection; Galactic chemical evolution; Radiative transfer; Stellar abundances; Stellar atmospheres; Stellar nucleosynthesis
dc.titleNew light on stellar abundance analyses: Departures from LTE and homogeneity.
dc.typeJournal article
local.bibliographicCitation.lastpage530
local.bibliographicCitation.startpage481
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu4042723@anu.edu.au
local.contributor.authoruidAsplund, Martin, u4042723
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub8476
local.identifier.citationvolume43
local.identifier.doi10.1146/annurev.astro.42.053102.134001
local.identifier.scopusID2-s2.0-26844559057
local.identifier.uidSubmittedByMigrated
local.type.statusPublished Version

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