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On the evolution of simulated galaxies: the mass dependence in metallicity gradients

Published online by Cambridge University Press:  21 March 2017

Maider Miranda ,
Patricia Sánchez-Blázquez ,
Chris B. Brook  and
Brad K. Gibson
Maider Miranda
Affiliation:
University of Central Lancashire, Preston, UK email: msancho@uclan.ac.uk Universidad Autónoma de Madrid, Madrid, Spain
Patricia Sánchez-Blázquez
Affiliation:
Universidad Autónoma de Madrid, Madrid, Spain
Chris B. Brook
Affiliation:
Universidad Autónoma de Madrid, Madrid, Spain
Brad K. Gibson
Affiliation:
University of Central Lancashire, Preston, UK email: msancho@uclan.ac.uk University of Hull, Hull, UK
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Making use of a fiducial set of simulated disc galaxies spanning a wide range of mass, we examine the influence of stellar mass in the radial metallicity gradients and compare to observational trends from Ho et al. (2015).

References

Brook, C. B., Stinson, G., Gibson, B. K., Wadsley, J., & Quinn, T. 2012, MNRAS, 424, 1275 CrossRefGoogle Scholar
Ho, I.-T., Kudritzki, R.-P., Kewley, L. J., Zahid, H. J., et al. 2015, MNRAS, 448, 2030 Google Scholar
Obreja, A., Brook, C. B., Stinson, G., Domínguez-Tenreiro, R., et al. 2014, MNRAS, 442, 1794 Google Scholar
Pilkington, K., Gibson, B. K., Brook, C. B., Calura, F., et al. 2012, MNRAS, 425, 969 Google Scholar