Channelled versus Isotropic Accretion of Galaxy Groups onto Clusters: Kinematics, Spin Alignment, and Assembly Bias
Published in MNRAS, accepted, 2026, 2026
How the route a galaxy group takes into a cluster, along a filament or from the open field, shapes its spin, kinematics and orbit, measured across 212,704 group-cluster infall pairs in the MDPL2 simulation.
Recommended citation: Singh A., Pearce F., Gray M., Kuchner U., Onions J., Yepes G., Knebe A., 2026, "Channelled versus Isotropic Accretion of Galaxy Groups onto Clusters: Kinematics, Spin Alignment, and Assembly Bias", MNRAS, accepted, arXiv:2610.39987. https://arxiv.org/abs/2610.39987
