The ODYSSEUS Survey. Spatial correlation of magnetospheric inclinations points to parsec-scale star-cloud connection
Caeley V. Pittman, Catherine C. Espaillat, Thanawuth Thanathibodee, Nuria Calvet, Lee W. Hartmann, Sylvie Cabrit

TL;DR
This study provides the first evidence of parsec-scale spatial correlations in stellar magnetospheric inclinations within a star-forming region, linking large-scale cloud structures to star system configurations.
Contribution
It introduces a novel analysis of spatial correlations of stellar inclinations at parsec scales, revealing a connection between large-scale cloud forces and star system orientations.
Findings
Magnetospheric inclinations are correlated over ~3 parsecs.
Spatial dependencies are stable against measurement uncertainties.
Lupus region shows non-uniform inclination distribution linked to filamentary structures.
Abstract
The properties of stars and planets are shaped by the initial conditions of their natal clouds. However, the spatial scales over which the initial conditions can exert a significant influence are not well constrained. We report the first evidence for parsec-scale spatial correlations of stellar magnetospheric inclinations (), observed in the Lupus low-mass star forming region. Applying consensus clustering with a hierarchical density-based clustering algorithm, we demonstrate that the detected spatial dependencies are stable against perturbations by measurement uncertainties. The correlation scales are on the order of ~3 pc, which aligns with the typical scales of the Lupus molecular cloud filaments. Our results reveal a connection between large-scale forces -- in the form of expanding shells from the Upper Scorpius and Upper-Centaurus-Lupus regions -- and…
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