Metallicity gradient of the thick disc progenitor at high redshift
We have developed a novel Markov Chain Mote Carlo (MCMC) 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...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
2017
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1706.01474
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| Author Notes: | 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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