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Scattering by Interstellar Dust Grains. I. Optical and Ultraviolet

  • Authors: B. T. Draine

Draine 2003 The Astrophysical Journal 598 1017.

  • Provider: AAS Journals

Caption: Fig. 5.

Degree of polarization as a function of scattering angle θ for scattering by Milky Way dust with ﹩R_{V}=3.1﹩, LMC average dust, and SMC bar dust. Curves are labeled by wavelength λ.

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