no code implementations • 5 Feb 2014 • Yohan Dubois, Christophe Pichon, Charlotte Welker, Damien Le Borgne, Julien Devriendt, Clotilde Laigle, Sandrine Codis, Dmitry Pogosyan, Stéphane Arnouts, Karim Benabed, Emmanuel Bertin, Jeremy Blaizot, François Bouchet, Jean-François Cardoso, Stéphane Colombi, Valérie de Lapparent, Vincent Desjacques, Raphaël Gavazzi, Susan Kassin, Taysun Kimm, Henry McCracken, Bruno Milliard, Sébastien Peirani, Simon Prunet, Stéphane Rouberol, Joseph Silk, Adrianne Slyz, Thierry Sousbie, Romain Teyssier, Laurence Tresse, Marie Treyer, Didier Vibert, Marta Volonteri
A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments above redshift 1. 2.
Cosmology and Nongalactic Astrophysics
no code implementations • 25 Jan 2018 • Nora Elisa Chisari, Mark L. A. Richardson, Julien Devriendt, Yohan Dubois, Aurel Schneider, Amandine M. C. Le Brun, Ricarda S. Beckmann, Sebastien Peirani, Adrianne Slyz, Christophe Pichon
Correspondingly, our results suggest that AGN feedback is not strong enough in the simulation.
Cosmology and Nongalactic Astrophysics
1 code implementation • 4 Jan 2019 • Thomas P. Galligan, Harley Katz, Taysun Kimm, Joakim Rosdahl, Jeremy Blaizot, Julien Devriendt, Adrianne Slyz
We show that the circumgalactic medium and diffuse gas surrounding the central regions of a galaxy are most affected by the interplay of radiation and gas, and that standard cooling functions that ignore the local radiation field can incorrectly predict the cooling rate by more than an order of magnitude, indicating that the baryon cycle in galaxies is affected by the influence of a local radiation field on the cooling rate.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
no code implementations • 2 Jul 2020 • Deaglan J. Bartlett, Harry Desmond, Julien Devriendt, Pedro G. Ferreira, Adrianne Slyz
We study the displacements between the centres of galaxies and their supermassive black holes (BHs) in the cosmological hydrodynamical simulation Horizon-AGN, and in a variety of observations from the literature.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
no code implementations • 4 Jan 2021 • Marius Ramsøy, Adrianne Slyz, Julien Devriendt, Clotilde Laigle, Yohan Dubois
At high redshift, the cosmic web is widely expected to have a significant impact on the morphologies, dynamics and star formation rates of the galaxies embedded within it, underscoring the need for a comprehensive study of the properties of such a filamentary network.
Astrophysics of Galaxies