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

Published online by Cambridge University Press:  17 July 2013

E. Ricciardelli ,
J. Navarro-González ,
V. Quilis  and
A. Vazdekis
E. Ricciardelli
Affiliation:
Departament d'Astronomia i Astrofisica, Universitat de Valencia, c/ Dr. Moliner 50, E-46100 - Burjassot, Valencia, Spain, email: [email protected]
J. Navarro-González
Affiliation:
Departament d'Astronomia i Astrofisica, Universitat de Valencia, c/ Dr. Moliner 50, E-46100 - Burjassot, Valencia, Spain, email: [email protected]
V. Quilis
Affiliation:
Departament d'Astronomia i Astrofisica, Universitat de Valencia, c/ Dr. Moliner 50, E-46100 - Burjassot, Valencia, Spain, email: [email protected]
A. Vazdekis
Affiliation:
Instituto de Astrofísica de Canarias, Vía Lactea s/n, E-38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, E-38205, Tenerife, Spain
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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).

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 366
Copyright
Copyright © International Astronomical Union 2013 

References

Quilis, V. 2004, MNRAS, 352, 1426Google Scholar
Ricciardelli, E., Vazdekis, A., Cenarro, A. J., & Falcón-Barroso, J. 2012, MNRAS, 424, 172Google Scholar
Vazdekis, A., Ricciardelli, E., Cenarro, A. J., et al. 2012, MNRAS, 424, 157Google Scholar