KRATOS: A large suite of N-body simulations to interpret the stellar kinematics of LMC-like discs
This collection of images shows different visualizations of the KRATOS suite. The main objective of these pure N-body simulations is to provide theoretical models that help us to interpret the formation of general structures in an LMC-like galaxy under various tidal interaction scenarios. For more information about the suite, we recomend reading the main reference (Jiménez-Arranz+24b).
The simulations are open access. Users interested in using the KRATOS suite of simulations can access them at:
https://dataverse.csuc.cat/dataset.xhtml?persistentId=doi:10.34810/data1156.