Flows around galaxies - I. The dependence of galaxy connectivity on cosmic environments and effects on the star formation rate

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Fig. 3.

Cosmic filaments (black lines) of the full TNG50-1 simulation. The red dots show the position of clusters of galaxies, i.e. the FoF haloes with masses M₂₀₀ > 10¹² M_⊙/h. The blue stars correspond to the 2942 central galaxies analysed in this work. The detection of the cosmic skeleton is presented in Sect. 3.3.

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