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Angle-dependent radiative grain alignment - Confirmation of a magnetic field – radiation anisotropy angle dependence on the efficiency of interstellar grain alignment | Astronomy & Astrophysics (A&A)
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Fig. 4

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The heating of asymmetrical grains, aligned with the magnetic field (thin, gray, lines) will vary with the angle Ψ. If only a fraction of the grains are alignable, we can use the variations in the dust temperature to estimate the fraction of aligned grains or the axes ratio of these asymmetric grains.

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