2010/09/22 by Andre L. B. Ribeiro, A. L. B. Ribeiro, Paulo A. A. Lopes +2
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Equipartition theorem #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Galaxy group #Gaussian #Physics #Quantum mechanics #RADIUS #Redshift #Stellar, planetary, and galactic studies #astro-ph.CO
paper · pdf · doi:10.1111/j.1745-3933.2010.00962.x
5 pages, 4 figures, accepted for publication in the MNRAS Letters
arxiv created 2010/09/22 · openalex publication_date 2010/10/12 · arxiv updated 2015/05/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Abstract We study segregation phenomena in 57 groups selected from the 2dF Percolation-Inferred Galaxy Groups (2PIGG) catalogue of galaxy groups. The sample corresponds to those systems located in areas of at least 80 per cent redshift coverage out to 10 times the radius of the groups. The dynamical state of the galaxy systems was determined after studying their velocity distributions. We have used the Anderson–Darling test to distinguish relaxed and non-relaxed systems. This analysis indicates that 84 per cent of groups have galaxy velocities consistent with the normal distribution, while 16 per cent of them have more complex underlying distributions. Properties of the member galaxies are investigated taking into account this classification. Our results indicate that galaxies in Gaussian groups are significantly more evolved than galaxies in non-relaxed systems out to distances of ∼4R200, presenting significantly redder (B−R) colours. We also find evidence that galaxies with MR≤−21.5 in Gaussian groups are closer to the condition of energy equipartition.