6 papers
Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights
Maria Rah, Areg Mickaelian, Francesco Flammini Dotti +1
We present a statistical study of pulsars and millisecond pulsars (MSPs) based on multiwavelength observations in the Galactic Field and Globular Clusters. We examine their emissio…
Rapid formation of a very massive star >50000 and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
Marcelo C. Vergara, Abbas Askar, Albrecht W. H. Kamlah +15
Context. We present simulations of a massive young star cluster using \textsc{Nbody6++GPU} and \textsc{MOCCA}. The cluster is initially more compact than previously published model…
DRAGON-III simulation: modelling million-body globular and nuclear star clusters
Kai Wu, Philip Cho, Rainer Spurzem +3
As a continuation of DRAGON-II, we present the DRAGON-III project, which focuses on the simulations of million-body globular clusters and nuclear clusters over 10 Gyr. We report on…
Evolution of star clusters with initial bulk rotation via N-body simulations
Abylay Bissekenov, Xiaoying Pang, Albrecht Kamlah +6
Young star clusters can inherit bulk rotation from the molecular clouds from which they have formed. This rotation can affect the long-term evolution of a star cluster and its cons…
Formation and Evolution of Compact Binaries Containing Intermediate Mass Black Holes in Dense Star Clusters`
Seungjae Lee, Hyung Mok Lee, Ji-hoon Kim +3
We investigate the evolution of star clusters containing intermediate-mass black hole (IMBH) of to , focusing on the formation and evolution of IMBH-s…
Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS: I. Free-floating MLPs
Francesco Flammini Dotti, M. B. N. Kouwenhoven, Peter Berczik +2
Context. Low-mass bodies, such as comets, asteroids, planetesimals, and free-floating planets, are continuously injected into the intra-cluster environment after expulsion from the…