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20242026
most citedExploring the ultra-faint dwarf Bootes I using JWST and HST: Metallicity distribution and binaries

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astro-ph.HE20251 cited

SN 2024aecx: A double-peaked rapidly evolving Type IIb supernova at 11 Mpc

Xingzhu Zou, Brajesh Kumar, Rishabh Singh Teja +28

We present the results of low-resolution spectroscopic and densely sampled multi-band photometric follow-up of supernova (SN) 2024aecx. The SN was discovered in the spiral galaxy N…

astro-ph.GA2025

Tracing ωCentauri's origins: Spatial and chemical signatures of its formation history

E. Dondoglio, A. P. Milone, A. F. Marino +8

ω}Centauri (ωCen) is the most enigmatic Galactic globular cluster (GC), with unmatched chemical complexity. We combine photometric and spectroscopic catalogs to identify its dist…

astro-ph.GA2025

The Small Magellanic Cloud through the lens of the James Webb Space Telescope : binaries and mass function within the galaxy outskirts

M. V. Legnardi, F. Muratore, A. P. Milone +8

The stellar initial mass function (IMF) and the fraction of binary systems are fundamental ingredients that govern the formation and evolution of galaxies. Whether the IMF is unive…

astro-ph.SR2025

Hunting for UVdim stars in Galactic Open clusters. Clues from ultraviolet photometry

G. Cordoni, A. P. Milone, L. Casagrande +7

Split main-sequences (MSs) and extended main-sequence turn-offs (eMSTOs) have been observed in nearly all Magellanic Clouds clusters younger than 2 Gyr. More recently, Hubble Space…

astro-ph.SR2025

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

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…