Galaxy Evolution in the context of radial metallicity gradients

Patricia B. Tissera

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

Resumen

The chemical abundances of the gas-phase and stellar components of disc galaxies are relevant to understand their formation and evolution. It has been shown that an inside-out disc formation yields negative chemical profiles. However, a large spread in metallicity gradients, including positive ones, has been reported by recent and more precise observations, suggesting the action of other physics processes such as gas outflows and inflows, radial migration, and mergers and interactions. Cosmological simulations that includes chemical models provide a tools to tackle the origin of the metallicity profiles and the action of those processes that might affect them as a function of time. I present a summary of the current state-of-knowledge from a numerical point of view and discuss the main results from the analysis of the EAGLE simulations.

Idioma originalInglés
Páginas (desde-hasta)255-256
Número de páginas2
PublicaciónProceedings of the International Astronomical Union
Volumen14
N.ºA30
DOI
EstadoPublicada - 1 ene 2018

Áreas temáticas de ASJC Scopus

  • Medicina (miscelánea)
  • Astronomía y astrofísica
  • Nutrición y dietética
  • Salud pública, medioambiental y laboral
  • Ciencias planetarias y espacial

Huella Profundice en los temas de investigación de 'Galaxy Evolution in the context of radial metallicity gradients'. En conjunto forman una huella única.

Citar esto