From roberto.capuzzodolcetta at uniroma1.it  Sat Jun  1 18:16:51 2019
From: roberto.capuzzodolcetta at uniroma1.it (Roberto Capuzzodolcetta)
Date: Sat, 1 Jun 2019 18:16:51 +0200
Subject: [astroseminar@Sapienza] seminario di astrofisica lunedi 3 giugno
	ore 16, aula Conversi
Message-ID: <CAMKCkgcd1L7-mKvM6eEF_YJ7paPYjZKzWkqwqE5yZhSioC0oTw@mail.gmail.com>

Ricordo il seminario di M. Fellhauer (Univ. de Concepcion, Cile),

- lunedi prossimo 3 giugno alle 16 in aula Conversi.

Title: How to form a dwarf spheroidal galaxy

Abstract: 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 explain our in situ models in more
detail. If time permits I will show how the dynamical properties of
dSph galaxies can be modeled without the need of DM or non-standard
gravity.


Reference advice: https://agenda.infn.it/event/18450/


-- 

Roberto CAPUZZO DOLCETTA  Roberto.Capuzzodolcetta at uniroma1.it
Dipartimento di Fisica, Universita' di Roma La Sapienza
P.le A.Moro 5, I-00185, Roma, Italy
Astronomy PhD program vice coordinator
phone: 39-06-49914535 fax:
39-06-4957697http://astrowww.phys.uniroma1.it/astro/dolcetta.html

-- 
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