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20162026
most citedDynamical Evolution of Multiple-Population Globular Clusters

54 citations · 110 across the 8 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

astro-ph.GA2024

MOCCA: Effects of pristine gas accretion and cluster migration on globular cluster evolution, global parameters, and multiple stellar populations

Mirek Giersz, Abbas Askar, Arkadiusz Hypki +3

Using the MOCCA code, we study the evolution of globular clusters (GCs) with multiple stellar populations. For this purpose, the MOCCA code has been significantly extended to take…

astro-ph.GA2024

Energy equipartition in multiple-population globular clusters

A. R. Livernois, F. I. Aros, E. Vesperini +7

We present the results of Monte Carlo simulations aimed at exploring the evolution towards energy equipartition of first- (1G) and second-generation (2G) stars in multiple-populati…

astro-ph.GA2024

Gravitational Wave Astronomy With TianQin

En-Kun Li, Shuai Liu, Alejandro Torres-Orjuela +50

The opening of the gravitational wave window has significantly enhanced our capacity to explore the universe's most extreme and dynamic sector. In the mHz frequency range, a divers…

astro-ph.GA2024

MOCCA: Global properties of tidally filling and underfilling globular star clusters with multiple stellar populations

Arkadiusz Hypki, Enrico Vesperini, Mirek Giersz +5

We explore the evolution of various properties of multiple-population globular clusters (GCs) for a broad range of initial conditions. We simulated over 200 GC models using the MOC…

astro-ph.SR2024

Double white dwarf binary population in MOCCA star clusters -- Comparisons with observations of close and wide binaries

Lucas Hellström, Mirosław Giersz, Arkadiusz Hypki +3

There could be a significant population of double white dwarf binaries (DWDs) inside globular clusters (GCs), however, these are often too faint to be individually observed. We hav…

astro-ph.GA2024

New Parameters for Star Cluster Dynamics: the role of clusters initial conditions

Bhavana Bhat, Barbara Lanzoni, Enrico Vesperini +4

We recently introduced three new parameters that describe the shape of the normalized cumulative radial distribution (nCRD) of the innermost stars in globular clusters and trace th…