Universality of dark matter haloes shape over six decades in mass: insights from the Millennium XXL and SBARBINE simulations

For the last 30 yr many observational and theoretical evidences have shown that galaxy clusters are not spherical objects, and that their shape is much better described by a triaxial geometry. With the advent of multiwavelength data of increasing quality, triaxial investigations of galaxy clusters i...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2015-05, Vol.449 (3), p.3171-3182
Hauptverfasser:	Bonamigo, Mario, Despali, Giulia, Limousin, Marceau, Angulo, Raul, Giocoli, Carlo, Soucail, Geneviève
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical instruments Astronomy Astrophysics Communities Computer simulation Cosmology Dark matter Galactic clusters Geometry Mathematical models Red shift Sciences of the Universe Simulation Stars & galaxies
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