A model for the post-collapse equilibrium of cosmological structure: Truncated isothermal spheres from top-hat density perturbations

Monthly Notices of the Royal Astronomical Society

Volumn 307, Issue 1, 1999, Pages 203-224

  Shapiro, Paul R ^a   Iliev, Ilian T ^b   Raga, Alejandro C ^c  

^a The University of Texas at Austin   (United States)

^b UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^c UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Cosmology: theory; Dark matter; Galaxies: clusters: general; Galaxies: formation; Galaxies: haloes; Galaxies: kinematics and dynamics

Indexed keywords

COSMOLOGY; GALAXIES; GRAVITATION; ISOTHERMS; KINEMATICS;

COSMOLOGY: THEORY; DARK MATTER; DENSITY PROFILE; GALAXIES: CLUSTERS: GENERAL; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY FORMATIONS; GALAXY:HALO; ISOTHERMAL SPHERES; POST-COLLAPSE; TOP HAT;

SPHERES;

EID: 0000995521     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02609.x     Document Type: Article

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