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The ODYSSEUS Survey. Spatial Correlation of Magnetospheric Inclinations Points to Parsec-scale Star–Cloud Connection

  • Authors: Caeley V. Pittman, Catherine C. Espaillat, Thanawuth Thanathibodee, Nuria Calvet, Lee W. Hartmann, Sylvie Cabrit

Caeley V. Pittman et al 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure 8.

Inclination uniformity test. Top: ﹩\cos ({i}_{{\rm{mag}}})﹩ histogram (left) and CDF (right) for the eight SFRs in C. V. Pittman et al. (2025a). The CDF figure shows the median and 95% confidence interval of the observed ﹩\cos ({i}_{{\rm{mag}}})﹩ values, as well as those of a uniform distribution. The observed ﹩\cos ({i}_{{\rm{mag}}})﹩ values are consistent with uniformity, within uncertainties. Bottom: same as the top panels, but for the Lupus sample in this work. These ﹩\cos ({i}_{{\rm{mag}}})﹩ values are inconsistent with uniformity.

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