Using observed total and polarized extinction curves, the paper derives a relation in which R_V varies from about 3.21 to 3.05 as the magnetic field moves from along the line of sight into the plane of the sky.
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The Optical Extinction Law Depends on Magnetic Field Orientation: The $R_V$-$\psi$ Relation
Using observed total and polarized extinction curves, the paper derives a relation in which R_V varies from about 3.21 to 3.05 as the magnetic field moves from along the line of sight into the plane of the sky.