output
20112025
most citedPre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency

36 citations

Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2024★ 14 cited

Abundance ties: Nephele and the globular cluster population accreted with Cen. Based on APOGEE DR17 and Gaia EDR3

Giulia Pagnini, Paola Di Matteo, Misha Haywood +8

The peculiar Galactic globular cluster Centauri (NGC 5139) has drawn attention for its unique features - such as a high stellar mass and a broad distribution of chemical elemen…

astro-ph.GA2024★ 17 cited

Simulating nearby disc galaxies on the main star formation sequence I. Bar formation and the building of the central gas reservoir

Pierrick Verwilghen, Eric Emsellem, Florent Renaud +14

Past studies have long emphasised the key role played by galactic stellar bars in the context of disc secular evolution, via the redistribution of gas and stars, the triggering of…

astro-ph.GA2024★ 15 cited

From giant clumps to clouds IV: extreme star-forming clumps on top of universal cloud scaling relations in gas-rich galaxies

Florent Renaud, Oscar Agertz, Alessandro B. Romeo

The clumpy nature of gas-rich galaxies at cosmic noon raises the question of universality of the scaling relations and average properties of the star-forming structures. Using cont…

astro-ph.GA2023★ 36 cited

Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency

Eric P. Andersson, Mordecai-Mark Mac Low, Oscar Agertz +2

The star cluster initial mass function is observed to have an inverse power law exponent around 2, yet there is no consensus on what determines this distribution, and why some vari…