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20072026
most citedDancing in the dark: galactic properties trace spin swings along the cosmic web

888 citations · 13.4k across the 233 of their papers we have counts for

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Showing 2018Show all

13 papers · 1 filter

astro-ph.GA2018★ 31 cited

Accurate tracer particles of baryon dynamics in the adaptive mesh refinement code Ramses

Corentin Cadiou, Yohan Dubois, Christophe Pichon

We present a new implementation of the tracer particles algorithm based on a Monte Carlo approach for the Eulerian adaptive mesh refinement code Ramses. The purpose of tracer parti…

astro-ph.GA2018★ 45 cited

Cosmic-ray propagation in the bi-stable interstellar medium. I. Conditions for cosmic-ray trapping

Benoît Commerçon, Alexandre Marcowith, Yohan Dubois

Cosmic rays (CR) propagate through the galactic scales down to the smaller scales at which stars form. CRs are close to energy equipartition with the other components of the inters…

astro-ph.GA2018★ 109 cited

Super-Eddington Accretion and Feedback from the First Massive Seed Black Holes

John A. Regan, Turlough P. Downes, Marta Volonteri +4

Super-Eddington accretion onto massive black hole seeds may be commonplace in the early Universe, where the conditions exist for rapid accretion. Direct collapse black holes are of…

astro-ph.GA2018★ 61 cited

Galaxies flowing in the oriented saddle frame of the cosmic web

K. Kraljic, C. Pichon, Y. Dubois +12

The strikingly anisotropic large-scale distribution of matter made of an extended network of voids delimited by sheets, themselves segmented by filaments, within which matter flows…

astro-ph.GA2018★ 39 cited

The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN

Mélanie Habouzit, Marta Volonteri, Rachel S. Somerville +4

High-redshift quasars are believed to reside in highly biased regions of the Universe, where black hole (BH) growth is sustained by an enhanced number of mergers and by being at th…

astro-ph.GA2018★ 93 cited

The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations

Jesse van de Sande, Claudia D. P. Lagos, Charlotte Welker +19

Cosmological hydrodynamical simulations are rich tools to understand the build-up of stellar mass and angular momentum in galaxies, but require some level of calibration to observa…