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19972026
most citedFormation and Dynamical Evolution of Multiple Stellar Generations in Globular Clusters

667 citations · 6.9k across the 171 of their papers we have counts for

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14 papers · 1 filter

astro-ph.GA2025★ 3 cited

Evolution of the kinematic properties of rotating multiple-population globular clusters

Ethan B. White, Enrico Vesperini, Emanuele Dalessandro +1

Globular clusters (GCs) host multiple stellar populations differing in their chemical and dynamical properties. A number of models for the formation of multiple populations predict…

astro-ph.SR2025

JWST imaging of omega Centauri: II. Evidence for a split white dwarf cooling sequence in the near-infrared

M. Scalco, M. Salaris, L. R. Bedin +11

We present a detailed analysis of the white dwarf cooling sequence (WD CS) in omega Centauri based on combined Hubble Space Telescope (HST) and JWST observations. Our analysis conf…

astro-ph.GA2025★ 1 cited

JWST imaging of omega Centauri -- I. Luminosity and mass functions of its main sequence populations

M. Scalco, R. Gerasimov, L. R. Bedin +10

This paper presents the first study of the most massive globular cluster (GC) in the Milky Way, omega Centauri, employing recently acquired JWST deep images. By combining these dat…

astro-ph.CO2025★ 5 cited

Dating N loud AGNs at high redshift: GS3073 as a snapshot of wCen like evolution of a nuclear star cluster

F. D'Antona, P. Ventura, A. F. Marino +8

In this paper we address two major questions raised by recent James Webb Space Telescope observations of the young Universe, namely: 1) what are the seed initial masses, and how ra…

astro-ph.SR2025★ 9 cited

A binary-related origin mediated by environmental conditions for blue straggler stars

Francesco R. Ferraro, Barbara Lanzoni, Enrico Vesperini +7

Blue stragglers are anomalously massive core hydrogen-burning stars that, according to the theory of single star evolution, should not exist. They are suspected to form in mass-enh…

astro-ph.GA2025★ 2 cited

Structural parameters, chronological age and dynamical age of the LMC globular cluster NGC 1754

Camilla Giusti, Mario Cadelano, Francesco R. Ferraro +4

In the context of a new systematic study of the properties of the most compact and massive star clusters in the Large Magellanic Cloud (LMC), here we present the determination of t…

astro-ph.GA2025★ 12 cited

SIEGE IV: compact star clusters in cosmological simulations with high star formation efficiency and sub-parsec resolution

R. Pascale, F. Calura, E. Vesperini +10

The formation of compact high-redshift star-forming clumps, the physical processes driving their evolution and their potential connection to present-day Globular Clusters are key o…

astro-ph.SR2025★ 4 cited

The internal kinematics of NGC 2808 and its multiple populations

M. Griggio, A. Bellini, F. I. Aros +10

We use new HST observations coupled with archival data spanning a total temporal baseline of 17 years to study the internal kinematics of the multiple populations in the globular c…

astro-ph.GA2025★ 6 cited

Phase-space mixing of multiple stellar populations in globular clusters

Francisco I. Aros, Enrico Vesperini, Emanuele Dalessandro

Context: Globular clusters (GCs) host multiple populations characterised by abundance variations in a number of light elements. In many cases, these populations also show spatial a…

astro-ph.GA2025

Tracing the W3/W4/W5 and Perseus complex dynamical evolution with star clusters

A. Della Croce, E. Dalessandro, E. Vesperini +4

The Perseus complex offers an ideal testbed to study cluster formation and early evolution as it hosts two major hierarchical structures (namely LISCA I and LISCA II) and the W3/W4…

astro-ph.SR2025★ 7 cited

A JWST project on 47 Tucanae. Binaries among multiple populations

A. P. Milone, A. F. Marino, M. Bernizzoni +25

Almost all globular clusters (GCs) contain multiple populations consisting of stars with varying helium and light-element abundances. These populations include first-population sta…

astro-ph.GA2025★ 9 cited

Exploring the formation environment of multiple stellar populations in Globular Clusters through binary systems

E. Bortolan, J. Bruce, A. P. Milone +9

Globular Clusters (GCs) are known to host distinct stellar populations, characterized by different chemical compositions. Despite extensive research, the origin of these population…

astro-ph.SR2025★ 5 cited

A JWST project on 47 Tucanae: kinematics, energy equipartition and anisotropy of multiple populations

T. Ziliotto, A. P. Milone, G. Cordoni +17

Recent work with JWST has demonstrated its capability to identify and chemically characterize multiple populations in globular clusters down to the H-burning limit. In this study,…

astro-ph.SR2025

JWST photometry and astrometry of 47 Tucanae. Discontinuity in the stellar sequence at the star/brown dwarf transition

M. Scalco, R. Gerasimov, L. R. Bedin +10

Using JWST Near Infrared Camera (NIRCam) images of the globular cluster 47 Tucanae (or NGC 104), taken at two epochs just 7 months apart, we derived proper-motion membership down t…