Hostname: page-component-6bf8c574d5-fppsw Total loading time: 0 Render date: 2025-02-14T12:44:39.280Z Has data issue: false hasContentIssue false
  • English
  • Français

Mirage simulations of the massiv sample

Published online by Cambridge University Press:  09 February 2015

P. Amram ,
V. Perret ,
B. Epinat ,
F. Bournaud ,
T. Contini ,
C. Divoy ,
B. Garilli ,
M. Kissler-Patig ,
O. Le Fevre  and
C. Lopez-Sanjuan
...Show all authors
P. Amram
Affiliation:
LAM, Marseille (F), Email: philippe.amram@lam.fr
V. Perret
Affiliation:
LAM, Marseille (F), Email: philippe.amram@lam.fr U. Zurich, (Ch)
B. Epinat
Affiliation:
LAM, Marseille (F), Email: philippe.amram@lam.fr
F. Bournaud
Affiliation:
CEA, SAp, AIM, Saclay(F)
T. Contini
Affiliation:
IRAP, Toulouse (F)
C. Divoy
Affiliation:
IRAP, Toulouse (F)
B. Garilli
Affiliation:
INAF-IASFBO, Bologna (I)
M. Kissler-Patig
Affiliation:
GEMINI, Hilo (USA)
O. Le Fevre
Affiliation:
LAM, Marseille (F), Email: philippe.amram@lam.fr
C. Lopez-Sanjuan
Affiliation:
FEFCA, Teruel(E)
J. Moultaka
Affiliation:
IRAP, Toulouse (F)
L. Pairo
Affiliation:
INAF-IASFBO, Bologna (I)
E. Perez-Montero
Affiliation:
IAC, Granada(E)
J. Queyrel
Affiliation:
IRAP, Toulouse (F)
L. Tasca
Affiliation:
LAM, Marseille (F), Email: philippe.amram@lam.fr
L. Tresse
Affiliation:
LAM, Marseille (F), Email: philippe.amram@lam.fr
D. Vergani
Affiliation:
INAF-IASF, Milano (I).
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 298
Copyright
Copyright © International Astronomical Union 2015