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Characterizing the hierarchical structure of filaments I. On the origin of the length-mass (L-M) scaling relation
Aims. Filamentary structures in molecular clouds are widely recognized as fundamental components of star formation. Observations report a length-mass relation of the form $L \propto M^α$ with $α\simeq 0.5$. We characterize this relation in simulated molecular clouds and investigate the influence of
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