Toward understanding rich superclusters
M. Einasto, E. Saar, V.J. Martinez, J. Einasto, L. J. Liivam"agi, E., Tago, J.-L. Starck, V. Mueller, P. Hein"am"aki, P. Nurmi, S. Paredes, M., Gramann, G. Huetsi

TL;DR
This study analyzes the structure and galaxy populations of two rich superclusters, revealing how local and global environments influence galaxy morphology, color, and evolution, with differences indicating distinct evolutionary histories.
Contribution
It provides a detailed morphological analysis of two superclusters using Minkowski functionals and galaxy group data, highlighting environmental effects on galaxy properties.
Findings
Core regions have more early-type, red galaxies and richer groups.
A morphological crossover occurs at a mass fraction of about 0.7.
Superclusters show different evolutionary histories.
Abstract
We present a morphological study of the two richest superclusters from the 2dF Galaxy Redshift Survey (SCL126, the Sloan Great Wall, and SCL9, the Sculptor supercluster). We use Minkowski functionals, shapefinders, and galaxy group information to study the substructure of these superclusters as formed by different populations of galaxies. We compare the properties of grouped and isolated galaxies in the core region and in the outskirts of superclusters. The fourth Minkowski functional and the morphological signature - show a crossover from low-density morphology (outskirts of supercluster) to high-density morphology (core of supercluster) at mass fraction . The galaxy content and the morphology of the galaxy populations in supercluster cores and outskirts is different. The core regions contain a larger fraction of early type, red galaxies, and richer…
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