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20132017
most citedMass models of NGC 6624 without an intermediate-mass black hole

47 citations · 56 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20179 cited

Three candidate double clusters in the LMC: truth or dare?

E. Dalessandro, A. Zocchi, A. L. Varri +6

The Large Magellanic Cloud (LMC) hosts a large number of candidate stellar cluster pairs. Binary stellar clusters provide important clues about cluster formation processes and the…

astro-ph.GA201747 cited

Mass models of NGC 6624 without an intermediate-mass black hole

Mark Gieles, Eduardo Balbinot, Rashid Yaaqib +4

An intermediate-mass black hole (IMBH) was recently reported to reside in the centre of the Galactic globular cluster (GC) NGC 6624, based on timing observations of a millisecond p…

astro-ph.GA2016

A class of spherical, truncated, anisotropic models for application to globular clusters

Ruggero de Vita, Giuseppe Bertin, Alice Zocchi

Recently, a class of non-truncated radially-anisotropic models (the so-called -models), originally constructed in the context of violent relaxation and modeling of ellipti…

astro-ph.SR2015

Biases in the determination of dynamical parameters of star clusters: today and in the Gaia era

A. Sollima, H. Baumgardt, A. Zocchi +4

The structural and dynamical properties of star clusters are generally derived by means of the comparison between steady-state analytic models and the available observables. With t…

astro-ph.GA2013

The flattening of globular clusters: internal rotation or velocity anisotropy?

Paolo Bianchini, Anna Lisa Varri, Giuseppe Bertin +1

Internal rotation is considered to play a major role in determining the structure and dynamics of some globular clusters. We present a dynamical analysis of the photometry and thre…