The first Giga-years of the Milky Way halo and its satellites told by RRLs

Autores
Giuliana Fiorentino
Fecha y hora
15 Sep 2022 - 11:30 Europe/London
Dirección

Pleyades

Idioma de la charla
Inglés
Idioma de la presentación
Inglés
Número en la serie
1
Descripción

The first Gigayears of our Galactic halo can be probed by using ancient stellar populations as traced by RR Lyrae stars. Today, with the advancement in our knowledge of RR Lyrae properties belonging to the Halo and to Milky Way satellite systems (Globular clusters and dwarf galaxies) we are able
to provide solid constraints on the link between these stellar systems. Here, we present some recent results concerning the Halo formation by using a detailed evolutionary analysis of RR Lyrae stars for which chemical abundances are available.

Tipo
SEVERO OCHOA