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Are “U-shape” age profiles a universal feature in spiral galaxies?

Published online by Cambridge University Press:  21 March 2017

Estrella Florido
Affiliation:
Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada, Spain. email: estrella@ugr.es, ruizlara@ugr.es, isa@ugr.es Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, E-18071
Tomás Ruiz-Lara
Affiliation:
Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada, Spain. email: estrella@ugr.es, ruizlara@ugr.es, isa@ugr.es Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, E-18071
Gareth Few
Affiliation:
School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, UK
Brad Gibson
Affiliation:
E.A. Milne Centre for Astrophysics, Department of Physics & Mathematics, University of Hull, Hull, HU6 7RX, UK
Isabel Pérez
Affiliation:
Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada, Spain. email: estrella@ugr.es, ruizlara@ugr.es, isa@ugr.es Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, E-18071
Ivan Minchev
Affiliation:
Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Patricia Sánchez-Blázquez
Affiliation:
Dpto. de Física Teórica, Universidad Autónoma de Madrid, E-28049 Cantoblanco, Spain
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In this work we study the effect of satellite accretion on the building-up of the radial stellar age distribution in the discs of spiral galaxies. In addition, we analyse its effect on other chemical and dynamical properties of these systems up to their outskirts.