36 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Institut de Recherche Mathématique AvancéeFR9 papers
- Centre National de la Recherche ScientifiqueFR4 papers
- Institute of Rural Management AnandIN4 papers
- Lund UniversitySE3 papers
- Observatoire astronomique de StrasbourgFR3 papers
- Université de StrasbourgFR3 papers
- Centre de Recherche en InformatiqueFR2 papers
- Gakushuin UniversityJP2 papers
- Tsinghua UniversityCN2 papers
- American Museum of Natural HistoryUS1 paper
- ARC Centre of Excellence for All-sky AstrophysicsAU1 paper
- Archéologie et Histoire Ancienne : Méditerranée – EuropeFR1 paper
4 papers · 1 filter
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…
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…
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…
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…