Astrofisica

# How to form a dSph galaxy

## by Michael Fellhauer (Departamento de Astronomia Universidad de Concepcion, Cile)

Europe/Rome
Aula Conversi (Dipartimento di Fisica - Ed. G. Marconi)

### Aula Conversi

#### Dipartimento di Fisica - Ed. G. Marconi

Description
I will review shortly the different models for the formation of dSph galaxies. We can differentiate three main pathways. One is the threshing and stripping scenario of larger systems. One is the pathway of in situ formation, i.e. they form as they appear now and the third possibility looks into a destroyed star cluster of tidal dwarf galaxy origin, i.e. without a DM halo. Our group has contributed models for the last two pathways and I will expl
Organized by

Roberto Capuzzo Docetta

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