activity
20152022
most citedA General Abundance Problem for All Self-Enrichment Scenarios for the Origin of Multiple Populations in Globular Clusters

134 citations · 617 across the 16 of their papers we have counts for

collaborators

28 papers

astro-ph.GA202225 cited

Deriving ages and horizontal branch properties of integrated stellar populations

Ivan Cabrera-Ziri, Charlie Conroy

A major source of uncertainty in the age determination of old ( Gyr) integrated stellar populations is the presence of hot horizontal branch (HB) stars. Here, we describe a…

astro-ph.SR202129 cited

Exploring the role of binarity in the origin of the bimodal rotational velocity distribution in stellar clusters

S. Kamann, N. Bastian, C. Usher +2

Many young and intermediate age massive stellar clusters host bimodal distributions in the rotation rates of their stellar populations, with a dominant peak of rapidly rotating sta…

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.SR20209 cited

Leveraging HST with MUSE: II. Na-abundance variations in intermediate age star clusters

S. Martocchia, S. Kamann, S. Saracino +13

Ancient (10 Gyr) globular clusters (GCs) show chemical abundance variations in the form of patterns among certain elements, e.g. N correlates with Na and anti-correlates with O.…

astro-ph.SR202017 cited

Leveraging HST with MUSE: I. Sodium abundance variations within the 2 Gyr-old cluster NGC 1978

S. Saracino, S. Kamann, C. Usher +10

Nearly all of the well studied ancient globular clusters (GCs), in the Milky Way and in nearby galaxies, show star-to-star variations in specific elements (e.g., He, C, N, O, Na, A…

astro-ph.GA202011 cited

Searching for globular cluster chemical anomalies on the main sequence of a young massive cluster

I. Cabrera-Ziri, J. S. Speagle, E. Dalessandro +9

The spectroscopic and photometric signals of the star-to-star abundance variations found in globular clusters seem to be correlated with global parameters like the cluster's metall…