activity
20062026
most citedThe Updated BaSTI Stellar Evolution Models and Isochrones: I. Solar Scaled Calculations

352 citations · 6.6k across the 189 of their papers we have counts for

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89 papers · 1 filter

astro-ph.SR2026

The variable mass-loss in low-mass red giant stars: Chromospheric motion across stellar evolution in 47 Tuc

Ian Baeza, L. Monaco, H. Frelijj +8

Mass-Loss (ML) is a critical process that remains poorly understood despite its broad implications across astrophysics. Our current knowledge is insufficient to reproduce ML consis…

astro-ph.SR2026

MINCE IV. A detailed analysis of 37 metal-poor and subsolar metallicity stars

L. Sgatti, G. Cescutti, L. Lombardo +13

The project called Measuring at Intermediate metallicity Neutron-Capture Elements (MINCE) primarily focuses on the photospheric abundances of several neutron-capture (NC) elements…

astro-ph.SR2026

X-shooter spectroscopy of giant stars in the nuclear star cluster

L. Origlia, C. Fanelli, A. Mucciarelli +5

Near-IR spectra of a homogeneous sample of 15 red giants in the Galactic nuclear star cluster, within 1.5 pc of SgrA*, have been acquired with X-shooter at the Very Large Telescope…

astro-ph.SR2026

Carbon measurements in two ultra-faint dwarf galaxies: Grus II and Tucana IV

Valentina Verdiani, Ása Skúladóttir, Romain Lucchesi +7

The ultra-faint dwarf galaxies (UFDs) are some of the oldest and most metal-poor environments in the Local Group. In particular, they are predicted to host the first stars (only H…

astro-ph.SR2026

MgAl burning chain in M 54: the globular cluster-like properties of a nuclear star cluster

D. A. Alvarez Garay, A. Mucciarelli, P. Ventura +2

In this study, we present the chemical abundances of Fe, Mg, Al, Si, and K for a sample of 233 likely member stars of M 54. All the stars were observed with the FLAMES high-resolut…

astro-ph.SR2025★ 2 cited

The chemical DNA of the Magellanic Clouds V. R-process dominates neutron capture elements production in the oldest SMC stars

Lorenzo Santarelli, Marco Palla, Alessio Mucciarelli +4

We present the chemical abundances of Fe, alpha- and neutron-capture elements in 12 metal-poor Small Magellanic Cloud (SMC) giant stars, observed with the high-resolution spectrogr…

astro-ph.SR2025

KOALA, a new ATLAS9 database -- I. Model atmospheres, opacities, fluxes, bolometric corrections, magnitudes and colours

A. Mucciarelli, P. Bonifacio, C. Lardo

We present the KOALA database, a new set of LTE, line-blanketed model atmospheres calculated with the code ATLAS9, together with the corresponding Opacity Distribution Functions an…

astro-ph.SR2025★ 1 cited

Fast Rotating Blue Straggler Stars in the globular cluster NGC 1851

Alex Billi, Lorenzo Monaco, Francesco R. Ferraro +4

In this work we study the rotational velocities of a sample of blue straggler stars (BSSs) and reference stars belonging to the Galactic globular cluster NGC 1851, using high-resol…

astro-ph.SR2025

The chemical DNA of the Magellanic Clouds III. The first, extragalactic Mg-K anticorrelation: the LMC globular cluster NGC 1786

Deimer Antonio Alvarez Garay, Alessio Mucciarelli, Lorenzo Monaco

In this work we derived [K/Fe] and [Mg/Fe] abundance ratios for six stars of the old globular cluster NGC 1786 in the Large Magellanic Cloud. We employed high-resolution spectra ac…

astro-ph.SR2025★ 3 cited

Detection of a white dwarf orbiting a Carbon-Oxygen depleted blue straggler in 47 Tucanae

Elisabetta Reggiani, Mario Cadelano, Barbara Lanzoni +3

We have employed deep far-UV observations secured with the Solar Blind Channel of the Advanced Camera for Surveys onboard the Hubble Space Telescope to search for hot companions to…

astro-ph.SR2025★ 2 cited

Inferring the efficiency of convective-envelope overshooting in Red Giant Branch stars

Lorenzo Briganti, Marco Tailo, Edoardo Ceccarelli +6

The understanding of mixing processes in stars is crucial for improving our knowledge of the chemical abundances in stellar photospheres and of their variation with evolutionary ph…

astro-ph.SR2024★ 5 cited

Rotational velocities of Blue Straggler Stars in the Globular Cluster M55

Alex Billi, Francesco R. Ferraro, Alessio Mucciarelli +3

By using high-resolution spectra acquired with FLAMES-GIRAFFE at the ESO/VLT, we measured radial and rotational velocities of 115 stars in the Galactic globular cluster M55. After…

astro-ph.SR2024★ 5 cited

The true nature of HE0057-5959, the most metal-poor Li-rich star

A. Mucciarelli, P. Bonifacio, L. Monaco +2

The Li-rich stars are a class of rare objects with A(Li) higher than that of other stars in the same evolutionary stage. Their origin is still debated and valuable routes are the C…

astro-ph.SR2024★ 1 cited

MINCE II. Neutron capture elements

P. François, G. Cescutti, P. Bonifacio +24

The MINCE (Measuring at Intermediate metallicity Neutron-Capture Elements) project aims to gather the abundances of neutron-capture elements but also of light elements and iron pea…

astro-ph.SR2024★ 5 cited

High speed stars: III. Detailed abundances and binary nature of the extreme speed star GHS143

E. Caffau, P. Bonifacio L. Monaco, L. Sbordone +7

The Gaia satellite has provided the community with three releases containing astrometrical and photometric data as well as by products, such as stellar parameters and variability i…

astro-ph.SR2023

The updated BaSTI stellar evolution models and isochrones.IV. alpha-depleted calculations

Adriano Pietrinferni, Maurizio Salaris, Santi Cassisi +4

This is the fourth paper of our new release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model and isochrone library. Following the updated solar-scaled, alpha-enh…

astro-ph.SR2023★ 23 cited

MgAl burning chain in Omega Centauri

Deimer Antonio Alvarez Garay, Alessio Mucciarelli, Michele Bellazzini +2

In this study, we report the results of Fe, Mg, Al, and Si abundances analysis for a sample of 439 stars in Omega Centauri, using high-resolution spectra obtained with the VLT/FLAM…

astro-ph.SR2023

Fast rotating Blue Straggler Stars in the Globular Cluster NGC3201

Alex Billi, Francesco R. Ferraro, Alessio Mucciarelli +7

We used high resolution spectra acquired at the Magellan Telescope to measure radial and rotational velocities of approximately 200 stars in the Galactic globular cluster NGC 3201.…

astro-ph.SR2023★ 31 cited

Fast rotating Blue Stragglers prefer loose clusters

Francesco R. Ferraro, Alessio Mucciarelli, Barbara Lanzoni +9

Blue stragglers are anomalously luminous core hydrogen-burning stars formed through mass-transfer in binary/triple systems and stellar collisions. Their physical and evolutionary p…

astro-ph.SR2022★ 21 cited

MINCE I. Presentation of the project and of the first year sample

G. Cescutti, P. Bonifacio, E. Caffau +20

In recent years, Galactic archaeology has become a particularly vibrant field of astronomy, with its main focus set on the oldest stars of our Galaxy. In most cases, these stars ha…

astro-ph.SR2022★ 133 cited

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products

G. Gilmore, S. Randich, C. C. Worley +165

The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representat…

astro-ph.SR2022★ 4 cited

Lithium detection in red supergiant stars of the Perseus complex

C. Fanelli, L. Origlia, A. Mucciarelli +3

We present the first systematic study of lithium abundance in a chemically homogeneous sample of 27 red supergiants (RSGs) in the young Perseus complex. For these stars, accurate s…

astro-ph.SR2022★ 29 cited

Discovery of a thin lithium plateau among metal-poor red giant branch stars

A. Mucciarelli, L. Monaco, P. Bonifacio +5

The surface lithium abundance A(Li) of warm metal-poor dwarf stars exhibits a narrow plateau down to [Fe/H]~-2.8 dex, while at lower metallicities the average value drops by 0.3 de…

astro-ph.SR2022★ 16 cited

The Mg-K anti-correlation in Omega Centauri

Deimer Antonio Alvarez Garay, Alessio Mucciarelli, Carmela Lardo +2

We present [K/Fe] abundance ratios for a sample of 450 stars in Omega Centauri, using high resolution spectra acquired with the multi-object spectrograph FLAMES@VLT. Abundances for…