The GALAH survey

verifying abundance trends in the open cluster M67 using non-LTE modelling

Xudong Gao*, Karin Lind, Anish M. Amarsi, Sven Buder, Aaron Dotter, Thomas Nordlander, Martin Asplund, Joss Bland-Hawthorn, Gayandhi M. De Silva, Valentina D'Orazi, Ken C. Freeman, Janez Kos, Geraint F. Lewis, Jane Lin, Sarah L. Martell, Katharine J. Schlesinger, Sanjib Sharma, Jeffrey D. Simpson, Daniel B. Zucker, Tomaž Zwitter & 10 others Gary Da Costa, Borja Anguiano, Jonathan Horner, Elaina A. Hyde, Prajwal R. Kafle, David M. Nataf, Warren Reid, Dennis Stello, Yuan Sen Ting, The GALAH collaboration

*Corresponding author for this work

Research output: Contribution to journalArticle

21 Citations (Scopus)
8 Downloads (Pure)

Abstract

Open cluster members are coeval and share the same initial bulk chemical composition. Consequently, differences in surface abundances between members of a cluster that are at different evolutionary stages can be used to study the effects of mixing and internal chemical processing. We carry out an abundance analysis of seven elements (Li, O, Na, Mg, Al, Si, and Fe) in 66 stars belonging to the open cluster M67, based on high resolution GALAH spectra, 1D MARCS model atmospheres, and non-local thermodynamic equilibrium (non-LTE) radiative transfer. From the non-LTE analysis, we find a typical star-to-star scatter in the abundance ratios of around 0.05 dex. We find trends in the abundance ratios with effective temperature, indicating systematic differences in the surface abundances between turn-off and giant stars; these trends are more pronounced when LTE is assumed. However, trends with effective temperature remain significant for Al and Si also in non-LTE. Finally, we compare the derived abundances with prediction from stellar evolution models including effects of atomic diffusion. We find overall good agreement for the abundance patterns of dwarfs and sub-giant stars, but the abundances of cool giants are lower relative to less evolved stars than predicted by the diffusion models, in particular for Mg.

Original languageEnglish
Pages (from-to)2666-2684
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Volume481
Issue number2
DOIs
Publication statusPublished - 1 Dec 2018

Bibliographical note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, Volume 481, Issue 2, December 2018, Pages 2666–2684, https://doi.org/10.1093/mnras/sty2414. Copyright 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Keywords

  • Radiative transfer
  • Stars: abundances
  • Stars: atmospheres
  • Stars: late-type

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