Structure and dynamics of massive galaxies at z=0 in a fully cosmological simulation

Bibcode
2013IAUS..295..366R
DOI
10.1017/S1743921313005383
Ricciardelli, E.; Navarro-González, J.; Quilis, V.; Vazdekis, A.
Referencia bibliográfica

The Intriguing Life of Massive Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 295, pp. 366-366

Fecha de publicación:
7
2013
Número de autores
4
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
In this contribution we present the results of an Eulerian adaptive mesh refinement (AMR) hydrodynamical and N-body simulation in a ΛCDM cosmology. The simulation used was performed with the cosmological code MASCLET (Quilis et al. 2004). Galaxies have been identified in the simulation outputs by means of an adaptive friends of friends algorithm applied to the star particles. To give light to our virtual galaxies we have assigned a spectrum to each stellar particle using the MIUSCAT stellar population models (Vazdekis et al. 2012; Ricciardelli et al. 2012).
Tipo
Sin árbitro

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