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The history of stellar metallicity in a simulated...
Journal article

The history of stellar metallicity in a simulated disc galaxy

Abstract

We explore the chemical distribution of stars in a simulated galaxy. Using simulations of the same initial conditions but with two different feedback schemes (McMaster Unbiased Galaxy Simulations – MUGS – and Making Galaxies in a Cosmological Context – MaGICC), we examine the features of the age–metallicity relation (AMR), and the three-dimensional age–[Fe/H]–[O/Fe] distribution, both for the galaxy as a whole and decomposed into disc, bulge, …

Authors

Snaith ON; Bailin J; Gibson BK; Bell EF; Stinson G; Valluri M; Wadsley J; Couchman H

Journal

Monthly Notices of the Royal Astronomical Society, Vol. 456, No. 3, pp. 3119–3141

Publisher

Oxford University Press (OUP)

Publication Date

March 1, 2016

DOI

10.1093/mnras/stv2788

ISSN

0035-8711