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20242026
most citedNowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST

1 citations · 2 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.GA20261 cited

Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST

Rupali Chandar, Miranda Caputo, Paul Goudfrooij +15

The Antennae galaxies merger produces the brightest infrared emission of any galaxy within ~20 Mpc, mostly from intense star formation taking place in supergiant molecular cloud co…

astro-ph.GA2026

Cosmic evolution of the [CII]-to-molecular gas relation

Cédric Accard, Florent Renaud, Katarina Kraljic +3

The [CII] 158 m line is widely used to trace star formation and the gas contents of high-redshift galaxies. However, it remains unclear under which physical conditions it relia…

astro-ph.GA20261 cited

The Nephele ecosystem: stars, globular clusters, and stellar streams associated with the progenitor galaxy of Centauri

G. Pagnini, P. Di Matteo, M. Haywood +7

Globular clusters (GCs) and their associated stellar streams are key tracers of the hierarchical assembly history of the Milky Way. Centauri, the most massive and chemically c…

astro-ph.GA2025

Asymmetries in stellar streams induced by a galactic merger

Claire Guillaume, Florent Renaud, Nicolas F. Martin +6

Stellar streams are sensitive to perturbations from, e.g., giant molecular clouds, bars and spiral arms, infalling dwarf galaxies, or globular clusters which can imprint gaps, clum…

astro-ph.GA2025

Forming the local starburst galaxy Haro 11 through hydrodynamical merger simulations

Timmy Ejdetjärn, Oscar Agertz, Florent Renaud +3

Haro 11 is a metal-poor, starburst galaxy believed to be the result of an ongoing merger, which is shaping the properties of the galaxy. In this study, we carry out a large suite o…

astro-ph.GA2025

Simulating nearby disc galaxies on the main star formation sequence II. The gas structure transition in low and high stellar mass discs

Pierrick Verwilghen, Eric Emsellem, Florent Renaud +14

Recent hydrodynamical simulations of isolated barred disc galaxies have suggested a structural change in the distribution of the interstellar medium (ISM) around a stellar mass M$_…