On the Dispersal of Young Stellar Hierarchies
Bruce G. Elmegreen

TL;DR
This paper investigates how young stellar hierarchies disperse over time, concluding that overlapping generations of star formation, rather than simple stellar motions or shear, primarily explain the disappearance of hierarchical structures.
Contribution
It introduces a model showing that overlapping star formation generations account for the dispersal of young stellar hierarchies, challenging previous explanations based on stellar motions or shear.
Findings
Hierarchical structures fade as multiple star formation generations overlap.
Power-law TPCFs persist during dispersal, indicating scale-independent mechanisms.
Overlapping generations reduce spatial correlations, explaining hierarchy disappearance.
Abstract
Hierarchical structure in young star fields has been demonstrated in a variety of ways, including two point correlation functions (TPCFs) that are power laws for spatial scales up to at least several hundred parsecs. As the stars age, this power law decreases in slope until it becomes nearly flat at ~100 Myr, at which point the hierarchical structure has disappeared. The fact that the TPCF remains nearly a power law during this time implies that the dispersal mechanism is somewhat independent of scale. This rules out dispersal by random stellar motions at either the local gas turbulent speed or a constant speed, because in both cases the hierarchy would disappear at small scales first, causing the TPCF to bend over. Destruction by shear has the right property as the shear rate in a galaxy is independent of scale for kpc-size regions, but shear converts the hierarchy into an azimuthal…
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