The GALAH survey: verifying abundance trends in the open cluster M67 using non-LTE modelling
ABSTRACT. Open cluster members are coeval and share the same initial bulk chemical composition. Consequently, differences in surface abundances between members
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 September 5
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 481, Heft: 2, Pages: 2666-2684 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2414 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1093/mnras/sty2414 Verlag: https://academic.oup.com/mnras/article/481/2/2666/5090981 
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| Verfasserangaben: | 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, Gary Da Costa, Borja Anguiano, Jonathan Horner, Elaina A. Hyde, Prajwal R. Kafle, David M. Nataf, Warren Reid, Dennis Stello, and Yuan-Sen Ting, the GALAH collaboration |
| Zusammenfassung: | ABSTRACT. Open cluster members are coeval and share the same initial bulk chemical composition. Consequently, differences in surface abundances between members |
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| Beschreibung: | Gesehen am 16.12.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2414 |