activity
20152021
most citedThe search for multiple populations in Magellanic Clouds clusters - V. Correlation between cluster age and abundance spreads

61 citations · 183 across the 7 of their papers we have counts for

collaborators

15 papers

astro-ph.GA20212 cited

Extragalactic globular clusters with Euclid and other wide surveys

Ariane Lançon, S. Larsen, K. Voggel +14

Globular clusters play a role in many areas of astrophysics, ranging from stellar physics to cosmology. New ground-based optical surveys complemented by observations from space-bas…

astro-ph.GA202114 cited

On the Nitrogen variation in ~2 Gyr old massive star clusters in the Large Magellanic Cloud

S. Martocchia, C. Lardo, M. Rejkuba +8

We present ESO/VLT FORS2 low resolution spectroscopy of red giant branch stars in three massive, intermediate age ( Gyr) star clusters in the Large Magellanic Cloud.…

astro-ph.SR2021

On the maximum helium content of multiple populations in the globular cluster NGC6752

Fabrice Martins, William Chantereau, Corinne Charbonnel

Multiple populations in globular clusters are usually explained by the formation of stars out of material with a chemical composition that is polluted to different degrees by the e…

astro-ph.SR2020

Searching for Multiple Populations in the Integrated Light of the Young and Extremely Massive Clusters in the Merger Remnant NGC~7252

Nate Bastian, Carmela Lardo, Christopher Usher +8

Recent work has shown that the properties of multiple populations within massive stellar clusters (i.e., in the extent of their abundance variations as well as the fraction of star…

astro-ph.SR2020

Chromosome maps of young LMC clusters: An additional case of coeval multiple populations

S. Saracino, S. Martocchia, N. Bastian +9

Recent studies have revealed that the Multiple Populations (MPs) phenomenon does not occur only in ancient and massive Galactic globular clusters (GCs), but it is also observed in…

astro-ph.GA202016 cited

The loss of the intra-cluster medium in globular clusters

W. Chantereau, P. Biernacki, M. Martig +3

Stars in globular clusters (GCs) lose a non negligible amount of mass during their post-main sequence evolution. This material is then expected to build up a substantial intra-clus…