Mass segregation and fractal substructure in young massive clusters – I. The McLuster code and method calibration

Mass segregation and fractal substructure in young massive clusters – I. The McLuster code and method calibration

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-11-01.

Descripteurs français

• Pascal (Inist)
  • Amas galaxies, Amas jeune, Amas stellaire, Analyse donnée, Couleur, Fonction masse, Fractal, Gradient densité, Gradient radial, Modèle 2 dimensions, Modèle amas, Modèle stellaire, Méthode gradient, Nuages Magellan, Paramètre s, Sous structure.

English descriptors

• KwdEn :
  • Aarseth, Absolute value, Algorithm, Ambiguous results, Andersen, Available code mcluster, Azimuthal, Azimuthal density, Azimuthal number density, Baumgardt, Binary, Binary pairing, Binary population, Binary systems, Bonnell, Brandl, Cambridge univ, Cartwright, Cartwright whitworth, Cent binaries, Central density, Centre, Cluster, Cluster centre, Cluster mass, Cluster model, Cluster stars, Color, Colour, Command line, Command line arguments, Computationally, Constituent stars, Crowther, Data analysis, Default, Density distribution, Density gradient, Different degrees, Dynamical, Edge length, Fractal, Fractal clusters, Fractal dimension, Fractal distribution, Fractal substructure, Gaburov gieles, Galaxy clusters, Gieles, Globular clusters, Goodwin, Gradient methods, Gutermuth, Heggie, High degree, High degrees, Highest degree, Hurley, Hydrodynamical computations, Initial conditions, Kick velocity, Kroupa, Ladislav subr, Local group, Local surface density, Local surface density measure, Lower values, Magellanic Clouds, Malumuth heap, Maschberger, Maschberger clarke, Mass function, Mass function slope, Mass function slope method, Mass limit, Mass segregation, Massive star, Massive stars, Mcluster, Mcluster code, Mcluster_sse, Metallicity, Mnras, Monthly notices, Multiple times, Nbody6, Observational data, Option, Pairing, Parameter, Parsec, Period distribution, Portegies, Portegies zwart, Pper, Quantifying, Quantifying mass segregation, Radial, Radial colour, Radial density, Radial density gradient, Radial distance, Radial gradient, Radial number density, Radial range, Radius, Random seed, Random subsets, S-parameters, Same mass, Sample size, Scale radius, Segregation, Selman, Similar mass companions, Solar units, Solid line, Standard deviation, Star, Star cluster, Star cluster formation, Star cluster models, Star clusters, Star formation, Star models, Stellar, Stellar evolution, Stellar mass, Stellar masses, Stellar populations, Stochastic scatter, Subr, Subset, Substructure, Substructured, Substructured models, Thermal eccentricity distribution, Total mass, Total number, Two dimensional model, Univ, Virial, Virial equilibrium, Whitworth, Young cluster, Young clusters, Young star clusters, Zwart.
• Teeft :
  • Aarseth, Absolute value, Algorithm, Ambiguous results, Andersen, Available code mcluster, Azimuthal, Azimuthal density, Azimuthal number density, Baumgardt, Binary, Binary pairing, Binary population, Binary systems, Bonnell, Brandl, Cambridge univ, Cartwright, Cartwright whitworth, Cent binaries, Central density, Centre, Cluster, Cluster centre, Cluster mass, Cluster stars, Colour, Command line, Command line arguments, Computationally, Constituent stars, Crowther, Default, Density distribution, Different degrees, Dynamical, Edge length, Fractal, Fractal clusters, Fractal dimension, Fractal distribution, Fractal substructure, Gaburov gieles, Gieles, Globular clusters, Goodwin, Gutermuth, Heggie, High degree, High degrees, Highest degree, Hurley, Hydrodynamical computations, Initial conditions, Kick velocity, Kroupa, Ladislav subr, Local group, Local surface density, Local surface density measure, Lower values, Malumuth heap, Maschberger, Maschberger clarke, Mass function, Mass function slope, Mass function slope method, Mass limit, Mass segregation, Massive star, Massive stars, Mcluster, Mcluster code, Mcluster_sse, Metallicity, Mnras, Monthly notices, Multiple times, Nbody6, Observational data, Option, Pairing, Parameter, Parsec, Period distribution, Portegies, Portegies zwart, Pper, Quantifying, Quantifying mass segregation, Radial, Radial colour, Radial density, Radial density gradient, Radial distance, Radial number density, Radial range, Radius, Random seed, Random subsets, Same mass, Sample size, Scale radius, Segregation, Selman, Similar mass companions, Solar units, Solid line, Standard deviation, Star, Star cluster, Star cluster formation, Star cluster models, Star clusters, Star formation, Stellar, Stellar evolution, Stellar mass, Stellar masses, Stellar populations, Stochastic scatter, Subr, Subset, Substructure, Substructured, Substructured models, Thermal eccentricity distribution, Total mass, Total number, Univ, Virial, Virial equilibrium, Whitworth, Young clusters, Young star clusters, Zwart.

Abstract

• https://api.istex.fr/document/B9F0A162848F4AFB168275C5B4397BB7B642466F/fulltext/pdf

Affiliations:

• Allemagne, Australie, Chili, France
• Auvergne-Rhône-Alpes, District de Cologne, Rhénanie-du-Nord-Westphalie, Rhône-Alpes
• Bonn, Grenoble

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