New light on stellar abundance analyses: Departures from LTE and homogeneity.
dc.contributor.author | Asplund, Martin | |
dc.date.accessioned | 2015-12-13T22:48:38Z | |
dc.date.issued | 2005 | |
dc.date.updated | 2015-12-11T10:29:40Z | |
dc.description.abstract | The 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.issn | 0066-4146 | |
dc.identifier.uri | http://hdl.handle.net/1885/80168 | |
dc.publisher | Annual Reviews Inc | |
dc.source | Annual Review of Astronomy and Astrophysics | |
dc.subject | Keywords: Convection; Galactic chemical evolution; Radiative transfer; Stellar abundances; Stellar atmospheres; Stellar nucleosynthesis | |
dc.title | New light on stellar abundance analyses: Departures from LTE and homogeneity. | |
dc.type | Journal article | |
local.bibliographicCitation.lastpage | 530 | |
local.bibliographicCitation.startpage | 481 | |
local.contributor.affiliation | Asplund, Martin, College of Physical and Mathematical Sciences, ANU | |
local.contributor.authoremail | u4042723@anu.edu.au | |
local.contributor.authoruid | Asplund, Martin, u4042723 | |
local.description.embargo | 2037-12-31 | |
local.description.notes | Imported from ARIES | |
local.description.refereed | Yes | |
local.identifier.absfor | 020110 - Stellar Astronomy and Planetary Systems | |
local.identifier.ariespublication | MigratedxPub8476 | |
local.identifier.citationvolume | 43 | |
local.identifier.doi | 10.1146/annurev.astro.42.053102.134001 | |
local.identifier.scopusID | 2-s2.0-26844559057 | |
local.identifier.uidSubmittedBy | Migrated | |
local.type.status | Published Version |
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