The use of supercomputers in stellar dynamics : proceedings of a workshop held at the Institute for Advanced Study, Princeton, USA, June 2-4, 1986

Gorde:
Xehetasun bibliografikoak
Erakunde egilea: Workshop on the use of supercomputers in stellar dynamics (Egilea)
Beste egile batzuk: McMillan, Stephen, 1955- (Argitalpenaren zuzendaria), Hut, Piet, 1952- (Argitalpenaren zuzendaria)
Formatua: Livre numérique
Hizkuntza:Anglais
Argitaratua: Berlin [etc.] : Springer [20..].
Cham : Springer Nature
Saila:Lecture notes in physics 267
Gaiak:
Sarrera elektronikoa:Accès sur la plateforme de l'éditeur
Accès sur la plateforme Istex
Accès Université d'Orléans
Accès INSA CVL
Oharra: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
Autres localisations: Voir dans le Sudoc
Edition sous un autre format:• The Use of supercomputers in stellar dynamics, proceedings of a workshop held at the Institute for Advanced Study, Princeton, USA, June 2-4, 1986, ed. by P. Hut and S. McMillan, Berlin, Springer-Verlag, 1986, 1 vol. (VI-240 p.), Lecture notes in physics, 3-540-17196-7
• The Use of Supercomputers in Stellar Dynamics, Texte imprimé, 9783662135808
• The Use of Supercomputers in Stellar Dynamics, Texte imprimé, 9783662135815
Aurkibidea:
  • Dynamical evolution of globular clusters
  • Disc galaxy dynamics on the computer
  • Star cluster dynamics: Mathematical models
  • Models of hot stellar systems
  • Supercomputers and large cosmological N-body simulations
  • Modelling stellar dynamical systems on the CRAY-1S and the CDC Cyber 205
  • Programming the ETA10 for large problems in stellar dynamics
  • The architecture of a homogeneous vector supercomputer
  • The BBN multiprocessors: Butterfly and Monarch
  • The Connection Machine
  • A digital Orrery
  • The outer solar system for 200 million years
  • Smooth particle hydrodynamics: Theory and application to the origin of the moon
  • Multiple mesh techniques for modelling interacting galaxies
  • Numerical experiments on galactic halo formation
  • Numerical integration using explicit taylor series
  • Multiple-mesh-particle scheme for N-body simulation
  • Direct N-body simulation on supercomputers
  • The vectorization of small-n integrators
  • N-body integrations using supercomputers
  • A new numerical technique for calculation of phase space evolution of stellar systems
  • An efficient N-body algorithm for a fine-grain parallel computer
  • A gridless fourier method
  • Techniques and tricks for N-body computation
  • On toolboxes and telescopes
  • A unified N-body method
  • Vectorization of N-body codes
  • Large scale calculations of core oscillations in globular clusters
  • Round-off sensitivity in the N-body problem
  • Formation of a bar through cold collapse of a stellar system
  • The gravitational interaction between N-body (star clusters) and hydrodynamic (ISM) codes in disk galaxy simulations
  • Standardised units and time scales.