In MHD cloud simulations, magnetic field geometry alone reduces the polarisation fraction of synthetic cold clumps by only about 1%, implying the larger observed drop towards real Planck clumps requires additional grain-alignment physics.
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Synthetic observations of dust emission and polarisation of Galactic cold clumps
In MHD cloud simulations, magnetic field geometry alone reduces the polarisation fraction of synthetic cold clumps by only about 1%, implying the larger observed drop towards real Planck clumps requires additional grain-alignment physics.