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Mirage simulations of the massiv sample

Amram, P. ; Perret, V. ; Epinat, B. ; Bournaud, F. ; Contini, T. ; Divoy, C. ; Garilli, B. ; Kissler-Patig, M. ; Le Fevre, O. ; Lopez-Sanjuan, C. ; Moultaka, J. ; Pairo, L. ; Perez-Montero, E. ; Queyrel, J. ; Tasca, L. ; Tresse, L. ; Vergani, D.

In: Proceedings of the International Astronomical Union, 2014, vol. 10, no. S309, p. 298-298

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    Titre
    • Mirage simulations of the massiv sample
    Auteur
    • Amram, P.. LAM, Marseille (F), Email: philippe.amram@lam.fr
    • Perret, V.. LAM, Marseille (F), Email: philippe.amram@lam.fr
    • Epinat, B.. LAM, Marseille (F), Email: philippe.amram@lam.fr
    • Bournaud, F.. CEA, SAp, AIM, Saclay(F)
    • Contini, T.. IRAP, Toulouse (F)
    • Divoy, C.. IRAP, Toulouse (F)
    • Garilli, B.. INAF-IASFBO, Bologna (I)
    • Kissler-Patig, M.. GEMINI, Hilo (USA)
    • Le Fevre, O.. LAM, Marseille (F), Email: philippe.amram@lam.fr
    • Lopez-Sanjuan, C.. FEFCA, Teruel(E)
    • Moultaka, J.. IRAP, Toulouse (F)
    • Pairo, L.. INAF-IASFBO, Bologna (I)
    • Perez-Montero, E.. IAC, Granada(E)
    • Queyrel, J.. IRAP, Toulouse (F)
    • Tasca, L.. LAM, Marseille (F), Email: philippe.amram@lam.fr
    • Tresse, L.. LAM, Marseille (F), Email: philippe.amram@lam.fr
    • Vergani, D.. INAF-IASF, Milano (I).
    Type de document
    • Postprint
    Langue
    • Anglais
    Publié dans
    • Proceedings of the International Astronomical Union, 2014, vol. 10, no. S309, p. 298-298. Cambridge University Press
    Autre version électronique
    Classification
    • Astronomie, Astrophysique
    Identifiant OAI-PMH
    • oai:doc.rero.ch:303271
    Summary
    The MIRAGE sample (Merging & isolated high-redshift AMR galaxies; Perret 2014, PhD dissertation; Perret et al. 2014, AA 562, 1) has been built in order to understand the contribution of the merger processes to the mass assembly in the MASSIV (Mass Assembly Survey with SINFONI in VVDS, Contini et al. 2012, AA 539, 91) sample. It consists of a sample of idealized simulations based on the RAMSES code; the initial conditions were designed to reproduce the physical properties of the most gas-rich young galaxies. The sample is composed of 20 simulations of mergers exploring the initial parameters of mass and orientation of the disks with a spatial resolution reaching 7 parsecs