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Aligned grains and scattered light found in gaps of planet-forming disk

Polarized (sub)millimetre emission from dust grains in circumstellar disks was initially thought to be because of grains aligned with the magnetic field1,2. However, higher-resolution multi-wavelength observations3–5 and improved models6–10 found that this polarization is dominated by self-scattering at shorter wavelengths (for example, 870 µm) and by grains aligned with something other than magnetic fields at longer wavelengths (for example, 3 mm). Nevertheless, the...
Monte Carlo Le Gouellec Gould Belt Distances Survey Astrophysics Source Code Library Long Baseline Campaign Belt Distances Survey
Source: nature.com

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