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20152026
most citedThe Accreted Nuclear Clusters of the Milky Way

82 citations · 822 across the 53 of their papers we have counts for

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21 papers · 1 filter

astro-ph.SR2026

The role of mass transfer efficiency in stability criteria: Implementation in SEVN and a test on blue stragglers and binary compact objects

M. Echeveste, G. J. Escobar, G. Iorio +12

Context: The stability of mass transfer through Roche-lobe overflow plays a key role in shaping the outcome of binary interactions. However, the criterion for mass transfer stabili…

astro-ph.SR2026

Stellar rotation and binaries in open clusters with Gaia DR3

Elena Pancino, Elisabetta Reggiani, Silvia Marinoni +14

Stellar rotation is a fundamental ingredient in shaping the evolution of stars and it can also be used to trace past stellar interactions. Yet, systematic studies of stellar rotati…

astro-ph.SR2025

Testing the Role of Merging Binaries in the Formation of the Split Main Sequence in Young Clusters

Nate Bastian, Sebastian Kamann, Florian Niederhofer +1

A number of theories have been put forward to explain the bi-modal stellar rotational distribution observed in young massive clusters. These include stellar mergers and interaction…

astro-ph.SR2025

Tracing stellar rotation in young massive LMC clusters

Sebastian Kamann, Nate Bastian, Florian Niederhofer +8

We present a detailed analysis of stellar rotation along the main sequences of NGC 1866 and NGC 1856, two young (~200-300 Myr) massive clusters in the Large Magellanic Cloud, using…

astro-ph.SR2025★ 2 cited

Survey of Surveys. II. Stellar parameters for 23 millions of stars

A. Turchi, E. Pancino, A. Avdeeva +16

In the current panorama of large surveys, the vast amount of data obtained with different methods, data types, formats, and stellar samples, is making an efficient use of the avail…

astro-ph.SR2024★ 12 cited

Binary properties of the globular cluster 47 Tuc (NGC 104). A dearth of short-period binaries

Johanna Müller-Horn, Fabian Göttgens, Stefan Dreizler +4

Spectroscopic observations of binary stars in globular clusters are essential to shed light on the poorly constrained period, eccentricity, and mass ratio distributions and to deve…

astro-ph.SR2023

Stellar Black Holes and Compact Stellar Remnants

Guglielmo Costa, Martyna Chruślińska, Jakub Klencki +4

The recent observations of gravitational waves (GWs) by the LIGO-Virgo-KAGRA collaboration (LVK) have provided a new opportunity for studying our Universe. By detecting several mer…

astro-ph.SR2023

A closer look at the binary content of NGC 1850

S. Saracino, S. Kamann, N. Bastian +7

Studies of young clusters have shown that a large fraction of O-/early B-type stars are in binary systems, where the binary fraction increases with mass. These massive stars are pr…

astro-ph.SR2023★ 14 cited

On the origin of UV-dim stars: a population of rapidly rotating shell stars?

Silvia Martocchia, Nate Bastian, Sara Saracino +1

The importance of stellar rotation in setting the observed properties of young star clusters has become clearer over the past decade, with rotation being identified as the main cau…

astro-ph.SR2022★ 40 cited

The effects of stellar rotation along the main sequence of the 100 Myr old massive cluster NGC 1850

Sebastian Kamann, Sara Saracino, Nate Bastian +13

Young star clusters enable us to study the effects of stellar rotation on an ensemble of stars of the same age and across a wide range in stellar mass and are therefore ideal targe…

astro-ph.SR2022★ 29 cited

Discovery of a double sequence of blue straggler stars in the core-collapsed globular cluster NGC 6256

Mario Cadelano, Francesco R. Ferraro, Emanuele Dalessandro +3

We used a combination of high-resolution optical images acquired with the Hubble Space Telescope and near-IR wide-field data to investigate the stellar density profile and the popu…

astro-ph.SR2021★ 29 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.SR2020★ 9 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.SR2020★ 17 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.SR2020★ 19 cited

Chromosome maps of young LMC clusters: An additional case of coeval multiple populations

S. Saracino, S. Martocchia, N. Bastian +9

Recent studies have revealed that the Multiple Populations (MPs) phenomenon does not occur only in ancient and massive Galactic globular clusters (GCs), but it is also observed in…

astro-ph.SR2019★ 17 cited

An Extragalactic Chromosome Map: The intermediate age SMC Cluster Lindsay 1

S. Saracino, N. Bastian, V. Kozhurina-Platais +8

The discovery of star-to-star abundance variations (a.k.a. multiple populations - MPs) within globular clusters (GCs), which are generally not found in the field or in lower mass o…

astro-ph.SR2019★ 20 cited

High-resolution extinction map in the direction of the bulge globular cluster NGC 6440

Cristina Pallanca, Francesco R. Ferraro, Barbara Lanzoni +3

We used optical images acquired with the UVIS channel of the Wide Field Camera 3 on board of the Hubble Space Telescope to construct the first high-resolution extinction map in the…

astro-ph.SR2018★ 27 cited

IC4499 revised: spectro-photometric evidence of small light-element variations

E. Dalessandro, C. Lardo, M. Cadelano +6

It has been suggested that IC4499 is one of the very few old globulars to not host multiple populations with light-element variations. To follow-up on this very interesting result,…

astro-ph.SR2018★ 12 cited

On the use of the main sequence knee (saddle) to measure globular cluster ages

S. Saracino, E. Dalessandro, F. R. Ferraro +11

In this paper we review the operational definition of the so-called main sequence knee (MS-knee), a feature in the color-magnitude diagram (CMD) occurring at the low-mass end of th…

astro-ph.SR2016★ 40 cited

Ultra-deep GEMINI near-infrared observations of the bulge globular cluster NGC 6624

S. Saracino, E. Dalessandro, F. R. Ferraro +8

We used ultra-deep and images secured with the near-infrared GSAOI camera assisted by the multi-conjugate adaptive optics system GeMS at the GEMINI South Telescope in Chi…

astro-ph.SR2015

GEMINI/GeMS observations unveil the structure of the heavily obscured globular cluster Liller 1

S. Saracino, E. Dalessandro, F. R. Ferraro +7

By exploiting the exceptional high-resolution capabilities of the near-IR camera GSAOI combined with the multi-conjugate adaptive optics system GeMS at the GEMINI South Telescope,…