activity
20082023
most citedThe long lives of giant clumps and the birth of outflows in gas-rich galaxies at high redshift

207 citations · 3.9k across the 83 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 119 cited

The origin of the Milky Way globular clusters

Florent Renaud, Oscar Agertz, Mark Gieles

We present a cosmological zoom-in simulation of a Milky Way-like galaxy used to explore the formation and evolution of star clusters. We investigate in particular the origin of the…

astro-ph.GA2016★ 127 cited

High-redshift major mergers weakly enhance star formation

J. Fensch, F. Renaud, F. Bournaud +11

Galaxy mergers are believed to trigger strong starbursts. This is well assessed by observations in the local Universe. However the efficiency of this mechanism has poorly been test…

astro-ph.GA2016★ 62 cited

Star formation triggered by galaxy interactions in modified gravity

Florent Renaud, Benoit Famaey, Pavel Kroupa

Together with interstellar turbulence, gravitation is one key player in star formation. It acts both at galactic scales in the assembly of gas into dense clouds, and inside those s…

astro-ph.GA2016★ 74 cited

The impact of stellar feedback on the density and velocity structure of the interstellar medium

Kearn Grisdale, Oscar Agertz, Alessandro B. Romeo +2

We study the impact of stellar feedback in shaping the density and velocity structure of neutral hydrogen (HI) in disc galaxies. For our analysis, we carry out pc resolut…

astro-ph.GA2016★ 78 cited

New insights on the formation of nuclear star clusters

Nicolas Guillard, Eric Emsellem, Florent Renaud

Nuclear Clusters (NCs) are common stellar systems in the centres of galaxies. Yet, the physical mechanisms involved in their formation are still debated. Using a parsec-resolution…

astro-ph.GA2016★ 62 cited

If it does not kill them, it makes them stronger: collisional evolution of star clusters with tidal shocks

Mark Gieles, Florent Renaud

The radii of young (<100 Myr) star clusters correlate only weakly with their masses. This shallow relation has been used to argue that impulsive tidal perturbations, or `shocks', b…