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Astrophysics and Space Science

, Volume 78, Issue 1, pp 145–156 | Cite as

Absorption bands and extinction in small interstellar particles

  • W. W. Duley
Article

Abstract

The production of discrete line and broad-band extinction by small interstellar oxide and silicate particles is discussed quantitatively. Restrictions on particle size and refractive index that are required to produce ‘pure’ absorption features are reviewed. The relationship between optical depth in interstellar extinction and absorption coefficients for bulk materials is used to reach some general conclusions concerning the diffuse interstellar features, VUV extinction and the composition of interstellar dust. It is noted that charge transfer bands of ions such as Fe3+ may be detectable in the VUV spectrum of dust. Several effects that lead to the enhancement of oscillator strength by 103–104 in small particles are discussed.

Keywords

Dust Optical Depth Mg2SiO4 Charge Transfer Band Interstellar Dust 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing 1981

Authors and Affiliations

  • W. W. Duley
    • 1
  1. 1.Physics DepartmentYork UniversityDownsviewCanada

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