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  1. Home
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Browsing by Author "Padilla, N"

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    Shapes of clusters and groups of galaxies
    (2006) Paz, DJ; Lambas, DG; Padilla, N; Merchán, M
    We study the properties of the three-dimensional and projected shapes of haloes using high-resolution numerical simulations and observational data where the latter comes from the 2PIGG [2dFGRS (2-degree Field Galaxy Redshift Survey) Percolation Inferred Galaxy Groups] and Data Release 3 of the Sloan Digital Sky Survey (SDSS-DR3GC) group catalogues. We investigate the dependence of the halo shape on characteristics such as mass and number of members. In the three-dimensional case, we find a significant correlation between the mass and the halo shape; massive systems are more prolate than small haloes. We detect a source of strong systematics in estimates of the triaxiality of a halo, which is found to be a strong function of the number of members; Lambda cold dark matter haloes usually characterized by triaxial shapes, slightly bent towards prolate forms, appear more oblate when taking only a small subset of the halo particles.

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