activity
20102026
most citedStar count density profiles and structural parameters of 26 Galactic globular clusters

140 citations · 1.8k across the 74 of their papers we have counts for

collaborators

78 papers

astro-ph.SR2026

Discovery of over a thousand variable stars in Terzan 5 and Liller 1 with JWST

Kevin B. Burdge, Ilaria Caiazzo, Malina M. Desai +18

The Bulge Fossil Fragments Terzan 5 and Liller 1 host some of the densest stellar environments in the Galaxy, yet their variable star populations have remained largely unexplored d…

astro-ph.HE2026

Discovery of the Infrared Counterpart of the Rapid Burster with JWST

Malina M. Desai, Kevin B. Burdge, Cristina Pallanca +8

The Rapid Burster (MXB 1730335) is the only known neutron star to produce both Type I and Type II X-ray bursts, making it a key system for understanding accretion physics onto n…

astro-ph.SR2026

The youngest white dwarf companion to a millisecond pulsar: Insights from NGC 362D

Greta Ettorre, Emanuele Dalessandro, Mario Cadelano +7

We report on the identification of the optical counterpart to the recently discovered millisecond pulsar (MSP) NGC362D in the Galactic globular cluster NGC362 based on deep, multi-…

astro-ph.HE2026

Exploring the optical properties of redback pulsars: The case of J1717+4308A in the globular cluster M92

Jianxing Chen, Greta Ettorre, Cristina Pallanca +13

Binary millisecond pulsars (MSPs) in globular clusters (GCs) are key for binary and stellar evolution studies under extreme conditions. The identification of their optical companio…

astro-ph.GA2026

CRIRES+ reveals the chemistry of the stellar sub-populations in the bulge fossil fragment Liller 1

L. Chiappino, L. Origlia, C. Fanelli +10

In this paper we present the chemical screening of the complex stellar population discovered in the Bulge Fossil Fragment Liller 1. This study is part of the Bulge Cluster Origin (…

astro-ph.HE2026

The one and the only: the pulsar - white dwarf system in NGC 6749

Paulo C. C. Freire, Yinfeng Dai, Mario Cadelano +7

PSR J1905+0154A is a binary millisecond pulsar located in the globular cluster (GC) NGC 6749. It was discovered in 2004 in a search for pulsars in GCs carried out with the Arecibo…

astro-ph.GA2026

The Bulge Cluster Origin (BulCO) survey with CRIRES at the ESO-VLT: a chemical screening of the Globular Cluster NGC 6553

A. Bartolomei, L. Origlia, C. Fanelli +10

In this paper we present the chemical screening of the stellar population belonging to the globular cluster NGC 6553 in the Galactic bulge. This study has been conducted in the con…

astro-ph.GA2026

Revealing the stellar population of the ultra-obscured Galactic globular cluster Glimpse-C02

M. Loriga, M. Cadelano, C. Pallanca +10

In this paper, we present the results of a detailed photometric analysis of Glimpse-C02, one of the most extincted globular clusters of the Milky Way. We built a deep color magnitu…

astro-ph.SR2025

A candidate to the long sought optical counterpart to the Rapid Burster in the bulge fossil fragment Liller 1

Cristina Pallanca, Francesco R. Ferraro, Barbara Lanzoni +6

We report on the possible identification of the optical counterpart of the Rapid Burster MXB 1730-335 in the stellar system Liller 1. The identification was performed by taking adv…

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.HE2025★ 4 cited

Searching for exotic object companions in the dense core of NGC 362: a multi-wavelength and multi-epoch photometric analysis

Greta Ettorre, Emanuele Dalessandro, Cristina Pallanca +8

The dense cores of globular clusters (GCs) are efficient environments for the production of exotic stellar populations, including millisecond pulsars (MSPs), low-mass X-ray binarie…

astro-ph.GA2025★ 7 cited

On the manifest link between Terzan 5 and the Galactic bulge

L. Origlia, F. R. Ferraro, C. Fanelli +4

We address the chemical link between Terzan 5 (hereafter Ter5) and the Bulge, as probed by the observed distributions of [/Fe] abundance ratios with varying [Fe/H] and by suitab…

astro-ph.GA2025★ 8 cited

The Bulge Cluster Origin (BulCO) survey at the ESO-VLT: probing the early history of the Milky Way assembling. Design and first results in Liller1

F. R. Ferraro, L. Chiappino, A. Bartolomei +14

We present the scientific goals and the very first results of the Bulge Cluster Origin (BulCO) survey. This survey has been specifically designed to perform an unprecedented chemic…

astro-ph.GA2025★ 5 cited

The bulge globular cluster Terzan 6 as seen from multi-conjugate adaptive optics and HST

Martina Loriga, Cristina Pallanca, Francesco R. Ferraro +7

This work consists of the first detailed photometric study of Terzan 6, one of the least known globular clusters in the Galactic bulge. Through the analysis of high angular resolut…

astro-ph.HE2025

Thirty-five years of timing of M53A with Arecibo and FAST

Yujie Lian, P. C. C. Freire, Shuo Cao +6

PSR B1310+18A is a 33-ms binary pulsar in a 256-day, low eccentricity orbit with a low-mass companion located in NGC 5024 (M53). In this Letter, we present the first phase-coherent…

astro-ph.GA2024

The star formation history of the first bulge fossil fragment candidate Terzan 5

Chiara Crociati, Michele Cignoni, Emanuele Dalessandro +6

Context. Terzan 5 and Liller 1 are the only bulge stellar clusters hosting multi-iron and multi-age stellar populations. They are therefore claimed to constitute a novel class of a…

astro-ph.GA2024

Multi-iron subpopulations in Liller 1 from high resolution H-band spectroscopy

C. Fanelli, L. Origlia, R. M. Rich +7

We present a high resolution chemical study of a representative sample of 21 luminous giant stars of Liller~1, a complex stellar system in the Galactic bulge, based on H band spect…

astro-ph.GA2024

Detailed chemical abundances of the globular cluster Terzan 6 in the inner bulge

C. Fanelli, L. Origlia, A. Mucciarelli +7

We used near-infrared spectroscopy at medium-high resolution (R=8,00025,000) to perform the first comprehensive chemical study of the intermediate luminosity bulge globular clus…

astro-ph.GA2024

The ESO-VLT MIKiS survey reloaded: the internal kinematics of the core of M75

Silvia Leanza, Cristina Pallanca, Francesco R. Ferraro +7

We present the results of a study aimed at characterizing the kinematics of the inner regions of the halo globular cluster M75 (NGC 6864) based on data acquired as part of the ESO-…

astro-ph.GA2024★ 5 cited

The dynamical age of the LMC globular cluster NGC 1835 using the "dynamical clock"

Camilla Giusti, Mario Cadelano, Francesco R. Ferraro +5

In the context of the study of the size-age relationship observed in star clusters in the Large Magellanic Cloud and the investigation of its origin, here we present the determinat…

astro-ph.GA2024

X-shooter spectroscopy of Liller1 giant stars

D. A. Alvarez Garay, C. Fanelli, L. Origlia +8

We present the first comprehensive chemical study of a representative sample of 27 luminous red giant branch (RGB) stars belonging to Liller 1, a complex stellar system in the Gala…

astro-ph.GA2024★ 4 cited

Discovery of an extended Horizontal Branch in the Large Magellanic Cloud globular cluster NGC1835

Camilla Giusti, Mario Cadelano, Francesco R. Ferraro +6

We present a high angular resolution multi-wavelength study of the massive globular cluster NGC 1835 in the Large Magellanic Cloud. Thanks to a combination of optical and near ultr…

astro-ph.HE2024★ 93 cited

A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes

Ewan D. Barr, Arunima Dutta, Paulo C. C. Freire +22

Among the compact objects observed in gravitational wave merger events a few have masses in the gap between the most massive neutron stars (NSs) and least massive black holes (BHs)…