Metallicity gradient of the thick disc progenitor at high redshift
We have developed a novel Markov Chain Monte Carlo chemical ‘painting’ technique to explore possible radial and vertical metallicity gradients for the thick disc progenitor. In our analysis, we match an N-body simulation to the data from the Apache Point Observatory Galactic Evolution Experiment sur...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 473, Heft: 1, Pages: 867-878 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx2464 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx2464 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/473/1/867/4222624 
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| Verfasserangaben: | Daisuke Kawata, Carlos Allende Prieto, Chris B. Brook, Luca Casagrande, Ioana Ciucă, Brad K. Gibson, Robert J.J. Grand, Michael R. Hayden and Jason A.S. Hunt |
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Metallicity gradient of the thick disc progenitor at high redshift
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