Gravitational clustering of galaxies : comparison between thermodynamic theory and N-body simulations. III: Velocity distributions for different mass components

Gravitational clustering of galaxies : comparison between thermodynamic theory and N-body simulations. III: Velocity distributions for different mass components

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Veröffentlicht in:The Astrophysical journal 1992-02, Vol.386 (1), p.9-18
Hauptverfasser: INAGAKI, S, ITOH, M, SASLAW, W. C
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Cosmology
Earth, ocean, space
Exact sciences and technology
Observational cosmology (including hubble constant, distance scale, cosmological constant, early universe, etc.)
Stellar systems. Galactic and extragalactic objects and systems. The universe
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doi_str_mv 10.1086/170986
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subjects Astronomy
Cosmology
Earth, ocean, space
Exact sciences and technology
Observational cosmology (including hubble constant, distance scale, cosmological constant, early universe, etc.)
Stellar systems. Galactic and extragalactic objects and systems. The universe
title Gravitational clustering of galaxies : comparison between thermodynamic theory and N-body simulations. III: Velocity distributions for different mass components
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