Image Details
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.
© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.