Showing 1–20 of 30 results
/ Date/ Name
Aug 30, 2010Compact Binaries in Star Clusters II - Escapers and Detection RatesJan 8, 2009Monte Carlo Simulations of Star Clusters - VI. The globular cluster NGC 6397Dec 28, 2006Dynamics of Planetary Systems in Star ClustersNov 16, 2007Modelling individual globular clustersFeb 24, 2025Multiple stellar populations in MOCCA globular cluster models: Transient spatial over-concentration of pristine red giant stars driven by strong dynamical encountersFeb 11, 2026Distance Estimation and Sky Localization of Eccentric Double White Dwarf Binaries from Gravitational Wave Observations inside Globular ClustersOct 3, 2009Compact Binaries in Star Clusters I - Black Hole Binaries Inside Globular ClustersJan 23, 2003Modest-2: A SummaryMay 9, 2022The impact of stellar evolution on rotating star clusters: the gravothermal-gravogyro catastrophe and the formation of a bar of black holesFeb 17, 2026Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problemFeb 6, 2026Exploring the dynamical evolution of binary stars in multiple-population globular clustersJun 7, 2022A Monte Carlo study of early gas expulsion and evolution of star clusters: new simulations with the MOCCA code in the AMUSE frameworkDec 4, 2013The M4 Core Project with HST --- I. Overview and First-EpochMar 19, 2024Discovery of a hot post-AGB star in Galactic globular cluster E3Jun 8, 2022MOCCA-Survey Database: Extra Galactic Globular Clusters. II. Milky Way and AndromedaJan 6, 2014The M4 Core Project with HST -- II. Multiple Stellar Populations at the Bottom of the Main SequenceFeb 4, 2018MOCCA-SURVEY Database I: Assessing GW kick retention fractions for BH-BH mergers in globular clustersJan 31, 2003A stochastic Monte Carlo approach to model real star cluster evolution, III. Direct integrations of three- and four-body interactionsDec 30, 2004Anisotropic gaseous models of tidally limited star clusters -- comparison with other methodsJun 21, 2017The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes