A three-component interstellar dust model with nanoparticles, amorphous grains, and micrometre-sized agglomerates using prolate shapes (axial ratio ~2), 10% porosity, and high alignment efficiency reproduces reddening and polarization spectra, with the large grains contributing one-third of visual 1
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Large Interstellar Polarisation Survey. III. Observational constraints on the structure of grains
A three-component interstellar dust model with nanoparticles, amorphous grains, and micrometre-sized agglomerates using prolate shapes (axial ratio ~2), 10% porosity, and high alignment efficiency reproduces reddening and polarization spectra, with the large grains contributing one-third of visual 1