most citedPulsars and Millisecond Pulsars II: Deep diving into the Evolutionary Mechanisms

2 citations · 3 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Simulating tidal disruption events in nuclear star clusters

Philip Cho, Kai Wu, Francesco Flammini Dotti +5

Context. Nuclear star clusters (NSCs) and supermassive black holes (SMBHs) often coexist at the centers of galaxies, engaging in complex dynamical interactions that influence SMBH…

astro-ph.HE2026★ 1 cited

Pulsars and Millisecond Pulsars III: Tracing Compact Object Dynamics in Globular Clusters with NBODY6++GPU

M. Rah, R. Spurzem, F. Flammini Dotti +1

Neutron stars in globular clusters follow complex evolutionary pathways shaped by binary interactions, mass transfer, and dynamical exchanges. Direct N-body simulations such as NBO…

astro-ph.GA2026

Modeling Tidal Disruption Events and Compact Object Plunges in Nuclear Star Clusters

Philip Cho, Kai Wu, Francesco Flammini Dotti +2

We study tidal disruption events (TDEs) and compact object inspirals in nuclear star clusters (NSCs) hosting a central supermassive black hole (SMBH), focusing on their role in SMB…

astro-ph.HE2026★ 2 cited

Pulsars and Millisecond Pulsars II: Deep diving into the Evolutionary Mechanisms

Maria Rah, Rainer Spurzem, Francesco Flammini Dotti +1

This second paper in our series investigates the evolutionary mechanisms that shape pulsars and millisecond pulsars (MSPs) across different astrophysical environments. We focus on…

astro-ph.IM2025

From Nbody1 to Nbody7: the Growth of Sverres Industry

Rainer Spurzem

From NBODY1 to NBODY6 : The Growth of an Industry is the title of a 1999 invited review by Sverre Aarseth, for Publications of the Astronomical Society of the Pacific (PASP). I too…

astro-ph.HE2025

Modelling Millisecond Pulsar Populations in Globular Clusters with NBODY6++GPU

Yuzhe Song, Debatri Chattopadhyay, Jarrod Hurley +3

Millisecond pulsars (MSPs) are neutron stars with spin periods as short as a few milliseconds, formed through mass accretion from companion stars. In the dense environments of glob…