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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

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Showing 2023Show all

11 papers · 1 filter

astro-ph.SR2023

EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey

M. G. Guarcello, E. Flaccomio, J. F. Albacete-Colombo +48

Context. With a mass exceeding several 10^4 solar masses and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming…

astro-ph.HE2023★ 16 cited

Discovery and Timing of Millisecond Pulsars in the Globular Cluster M5 (NGC 5904) with FAST and Arecibo

Lei Zhang, Paulo C. C. Freire, Alessandro Ridolfi +29

We report on a comprehensive multi-wavelength study of the pulsars in the globular cluster (GC) M5, including the discovery of M5G, a new compact non-eclipsing "black widow" pulsar…

astro-ph.GA2023★ 8 cited

A Photometric in-depth look at the core-collapsed globular cluster NGC 6284

Dan Deras, Mario Cadelano, Barbara Lanzoni +4

High-resolution Hubble Space Telescope (\textit{HST}) optical observations have been used to perform the deepest photometric study of the poorly studied Galactic globular cluster N…

astro-ph.GA2023★ 22 cited

JWST uncovers helium and water abundance variations in the bulge globular cluster NGC 6440

Mario Cadelano, Cristina Pallanca, Emanuele Dalessandro +9

We used ultra-deep observations obtained with the NIRCam aboard the James Webb Space Telescope to explore the stellar population of NGC 6440: a typical massive, obscured and contam…

astro-ph.GA2023★ 6 cited

An ongoing tidal capture in the Large Magellanic Cloud: the low-mass star cluster KMK88-10 captured by the massive globular cluster NGC 1835?

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

In the context of a project aimed at characterizing the dynamical evolution of old globular clusters in the Large Magellanic Cloud, we have secured deep HST/WFC3 images of the mass…

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.GA2023★ 27 cited

First evidence of multi-iron sub-populations in the Bulge Fossil Fragment candidate Liller 1

Chiara Crociati, Elena Valenti, Francesco R. Ferraro +8

In the context of a project aimed at characterizing the properties of the so-called Bulge Fossil Fragments (the fossil remnants of the bulge formation epoch), here we present the f…

astro-ph.SR2023★ 4 cited

The "canonical" White Dwarf Cooling Sequence of M5

Jianxing Chen, Francesco R. Ferraro, Maurizio Salaris +5

Recently, a new class of white dwarfs (dubbed ``slowly cooling WDs'') has been identified in two globular clusters (namely M13 and NGC 6752) showing a horizontal branch (HB) morpho…

astro-ph.GA2023★ 13 cited

Internal kinematics and structure of the bulge globular cluster NGC 6569

Cristina Pallanca, Silvia Leanza, Francesco R. Ferraro +8

In the context of a project aimed at characterizing the properties of star clusters in the Galactic bulge, here we present the determination of the internal kinematics and structur…

astro-ph.GA2023★ 19 cited

Empirical measurement of the dynamical ages of three globular clusters and some considerations on the use of the dynamical clock

Francesco R. Ferraro, Barbara Lanzoni, Enrico Vesperini +3

We have used the ``dynamical clock'' to measure the level of dynamical evolution reached by three Galactic globular clusters (namely, NGC 3201, NGC 6316 and NGC 6440). This is an e…

astro-ph.HE2023★ 11 cited

A young white dwarf orbiting PSR J1835-3259B in the bulge globular cluster NGC 6652

J. Chen, M. Cadelano, C. Pallanca +8

We report on the discovery of the companion star to the millisecond pulsar PSR J1835-3259B in the Galactic globular cluster NGC 6652. Taking advantage of deep photometric archival…