B-fields In STar-forming Region Observations (BISTRO): Population-Level Universality and Environmental Structuring of 450/850 m Polarization Signatures
arXiv:2611.10458
Abstract
We observed 69 molecular cloud regions at 450 and 850 m with the POL-2 polarimeter on the James Clerk Maxwell Telescope and matched the maps to a common beam. Polarization fractions are typically lower at 450 m. The median of 30 measured ratios is . Across 35 regions with reliable spectral indices of total () and polarized () intensity, the medians over sources are and -. The median is to , with in 24-27 regions. These ranges span the two extreme placements of limits for polarized intensity below the noise floor. The position angles at the two wavelengths agree within in 10 of 13 regional medians, disfavoring a geometric origin that would rotate the angles. The medians of in 9 low-mass, 19 high-mass and 7 Central Molecular Zone (CMZ) regions are not ordered low-mass high-mass CMZ (Jonckheere-Terpstra -). A difference among classes is not robustly detected. The Kruskal-Wallis - becomes - when the Rosette Molecular Cloud alone is excluded, although the high-mass class has the lowest median in every treatment. The classes follow a distance sequence (the beam spans 0.008-0.51 pc), coupling environment and physical scale. Within clouds, the 450 m polarization fraction decreases with Herschel column density in all 7 fields with sufficient dynamic range. Coefficients from pooled pixels mix trends within clouds, differences between clouds, and the influence of OMC 1. They therefore do not define a single law for individual pixels. The wavelength dependence across sources provides a benchmark for grain alignment. We cannot order it by environment and do not propose a unique mechanism.
arXiv comment161 pages, 88 figures, 21 tables. Submitted to PASJ. Paper S2 of a series of three (Papers T, S1, and S2); Papers T and S1 are arXiv:2610.29273 and arXiv:2610.29285. The submitted versions of all three papers are available at https://github.com/450um1G/PASJ2026