most citedDriving factors behind multiple populations

7 citations · 12 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025

Spectroscopic Confirmation: Fast rotators in the young clusters NGC 1856 and NGC 1953

Paul I. Cristofari, Andrea K. Dupree, Antonino P. Milone +2

We present the results of a spectroscopic investigation of two Large Magellanic Cloud globular clusters, NGC 1953 and NGC 1856. Both clusters have similar ages (250 and 300 Myr, re…

astro-ph.SR2025★ 4 cited

New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling

Irene Vargas-Salazar, M. S. Oey, Jan J. Eldridge +9

We present a radial velocity (RV) survey of the field OB and OBe stars of the SMC Wing. We use multi-epoch observations of 55 targets obtained with the Magellan IMACS and M2FS mult…

astro-ph.SR2024

Rotation and H emission in a young SMC cluster: a spectroscopic view of NGC 330

Paul I. Cristofari, Andrea K. Dupree, Antonino P. Milone +4

We present an analysis of high-resolution optical spectra recorded for 30 stars of the split extended main-sequence turnoff (eMSTO) of the young ( 40 Myr) Small Magellanic Cl…

astro-ph.SR2024★ 1 cited

Abundances of Neutron-Capture Elements in 62 Stars in the Globular Cluster Messier 15

Jonathan Cabrera Garcia, Charli M. Sakari, Ian U. Roederer +7

M15 is a globular cluster with a known spread in neutron-capture elements. This paper presents abundances of neutron-capture elements for 62 stars in M15. Spectra were obtained wit…

astro-ph.GA2024★ 7 cited

Driving factors behind multiple populations

Ruoyun Huang, Baitian Tang, Chengyuan Li +9

Star clusters were historically considered simple stellar populations, with all stars sharing the same age and initial chemical composition. However, the presence of chemical anoma…