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dc.contributor.authorZhao, G.
dc.contributor.authorMashonkina, L.
dc.contributor.authorYan, H. L.
dc.contributor.authorAlexeeva, S.
dc.contributor.authorKobayashi, C.
dc.contributor.authorPakhomov, Yu
dc.contributor.authorShi, J. R.
dc.contributor.authorSitnova, T.
dc.contributor.authorTan, K. F.
dc.contributor.authorZhang, H. W.
dc.contributor.authorZhang, J. B.
dc.contributor.authorZhou, Z. M.
dc.contributor.authorBolte, M.
dc.contributor.authorChen, Y. Q.
dc.contributor.authorLi, X.
dc.contributor.authorLiu, F.
dc.contributor.authorZhai, M.
dc.date.accessioned2017-06-15T14:42:20Z
dc.date.available2017-06-15T14:42:20Z
dc.date.issued2016-12-19
dc.identifier.citationZhao , G , Mashonkina , L , Yan , H L , Alexeeva , S , Kobayashi , C , Pakhomov , Y , Shi , J R , Sitnova , T , Tan , K F , Zhang , H W , Zhang , J B , Zhou , Z M , Bolte , M , Chen , Y Q , Li , X , Liu , F & Zhai , M 2016 , ' Systematic non-LTE study of the $-2.6 \le$ [Fe/H] $\le 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu ' The Astrophysical Journal , vol. 833 , no. 2 . https://doi.org/10.3847/1538-4357/833/2/225
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 10547815
dc.identifier.otherPURE UUID: e6078491-3b32-4319-af2c-5c054870de96
dc.identifier.otherArXiv: http://arxiv.org/abs/1610.00193v1
dc.identifier.otherScopus: 85007614063
dc.identifier.urihttp://hdl.handle.net/2299/18343
dc.descriptionG. Zhao, et al, 'SYSTEMATIC NON-LTE STUDY OF THE −2.6 „ [Fe/H] „ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. II. ABUNDANCE PATTERNS FROM Li TO Eu*', The Astrophysical Journal, Vol. 833 (2), December 2016, doi:10.3847/1538-4357/833/2/225. © 2016. The American Astronomical Society. All rights reserved.
dc.description.abstractFor the first time, we present an extensive study of stars with individual non-local thermodynamic equilibrium (NLTE) abundances for 17 chemical elements from Li to Eu in a sample of stars uniformly distributed over the $-2.62 \le$ [Fe/H] $\le +0.24$ metallicity range that is suitable for the Galactic chemical evolution research. The star sample has been kinematically selected to trace the Galactic thin and thick disks and halo. We find new and improve earlier results as follows. (i) The element-to-iron ratios for Mg, Si, Ca, and Ti form a MP plateau at a similar height of 0.3~dex, and the knee occurs at common [Fe/H] $\simeq -0.8$. The knee at the same metallicity is observed for [O/Fe], and the MP plateau is formed at [O/Fe] = 0.61. (ii) The upward trend of [C/O] with decreasing metallicity exists at [Fe/H] $$en
dc.format.extent26
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectgalaxy: evolution
dc.subjectline: formatin
dc.subjectstars: abundances
dc.subjectstars: atmospheres
dc.subjectstars: late-type
dc.titleSystematic non-LTE study of the $-2.6 \le$ [Fe/H] $\le 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Euen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttps://arxiv.org/abs/1610.00193
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2016-09-27
rioxxterms.versionAM
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.3847/1538-4357/833/2/225
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeopenAccess


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