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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. 10.

Scattering asymmetry factor ﹩g=\langle \mathrm{cos}\,\theta \rangle ﹩ as a function of frequency for different MW dust mixtures. Also shown are observational estimates for g in various regions. The values are from the following sources, as indicated in the figure: Schiminovich et al. (2001), Witt et al. (1982, 1990, 1992, 1997), Murthy & Henry (1995), Hurwitz et al. (1991), Lillie & Witt (1976), Mattila (1970), Gordon et al. (1994), Gibson & Nordsieck (2003), Burgh et al. (2002), and Calzetti et al. (1995).

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