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Black hole fuelling in galaxy mergers: a high-resolution analysis
(Oxford, 2021)
Using parsec scale resolution hydrodynamical adaptive mesh refinement simulations, we have studied the mass transport process throughout a Galactic merger. The aim of such study is to connect both the peaks of mass accretion ...
The evolution of the star formation rate function in the Eagle simulations: a comparison with UV, IR and H alpha observations from z ∼ to 8 to z ∼ to 0
(Oxford university press, 2017)
We investigate the evolution of the galaxy star formation rate function (SFRF) and cosmic star formation rate density (CSFRD) of z similar to 0-8 galaxies in the Evolution and Assembly of GaLaxies and their Environments ...
Simulaciones del proceso de formación de estrellas en galaxiasSimulations of Star Formation Process in Galaxies
(Sociedad Colombiana de FísicaGrupo de Física y Astrofísica Computacional (FACOM)Bogotá Colombia, 2021)
Angular momentum evolution for galaxies in a Λ-CDM scenario
(EDP Sciences, 2015-12)
Context. Galaxy formation in the current cosmological paradigm is a verycomplex process in which inflows, outflows, interactions, and mergersare common events. These processes can redistribute the angular momentumcontent ...
Fingerprints of the hierarchical building-up of the structure on the gas kinematics of galaxies
(EDP Sciences, 2012-10)
Context. Recent observational and theoretical works have suggested that the Tully-Fisher relation might be generalised to include dispersion-dominated systems by combining the rotation and dispersion velocity in the ...
Multiscale mass transport in z ∼6 galactic discs: fuelling black holes
(Royal Astronomical Society, 2016)
By using Adaptive Mesh Refinement cosmological hydrodynamic N-body zoom-in simulations,
with the RAMSES code, we studied the mass transport processes on to galactic nuclei
from high redshift up to z ∼6. Due to the large ...
GHASP: an H alpha kinematic survey of spiral and irregular galaxies - IX. The near-infrared, stellar and baryonic Tully-Fisher relations
(WILEY-BLACKWELL, 2011)
We studied, for the first time, the near-infrared, stellar and baryonic Tully-Fisher relations for a sample of field galaxies taken from a homogeneous Fabry-Perot sample of galaxies [the Gassendi HAlpha survey of SPirals ...
Morphology of galaxies with quiescent recent assembly history in a Λ-CDM universe
(EDP Sciences, 2014-07)
Context. The standard disc formation scenario postulates that the disc forms as the gas cools and flows into the centre of the dark matter halo, conserving the specific angular momentum. Major mergers have been shown to ...