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Structure and evolution of metallicity and age radial profiles in Milky-Way-like galaxies

Published online by Cambridge University Press:  03 March 2020

E. Athanassoula
E. Athanassoula*
Affiliation:
Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
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Abstract

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I will give here a very short summary of some of the work I have been doing lately on the chemical evolution in Milky-Way-like spiral galaxies.

Keywords

methods: n-body simulationsgalaxies: abundancesgalaxies: spiralgalaxies: evolutiongalaxies: structureGalaxy: abundancesGalaxy: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 284
Copyright
© International Astronomical Union 2020

References

Athanassoula, E. 2017, in IAU Symposium 321, Formation and Evolution of Galaxy Outskirts, ed. Gil de Paz, A., Knapen, J., Lee, J., (Cambridge: Cambridge Univ. Press), 61Google Scholar
Athanassoula, E., Rodionov, S., Peschken, N., Lambert, J.C. 2016, ApJ, 821, 90 CrossRefGoogle Scholar
Athanassoula, E., Rodionov, S., Prantzos, N. 2017, MNRAS, 467L, 46 CrossRefGoogle Scholar