BRILLO SUPERFICIAL, TAMAÑO, HISTORIA DE FORMACIÓN ESTELAR Y CINEMÁTICA DE GALAXIAS ENANAS SIMULADAS: EL IMPACTO DE LOS PARÁMETROS LIBRES DE LAS SIMULACIONES
According to the standard cosmological model, structure formation occurs in a bottom up fashion, where small galaxies are formed first while bigger systems grow by continuous aggregation of smaller ones. Both observations and theoretical predictions of the galaxy mass function agree on the fact that dwarfs are the most numerous galaxies in the
Salvador Cardona Barrero
Fecha de publicación:
3
2023