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Optical properties of interstellar graphite and silicate grains

Draine, B. T., Lee, H. M.·1984·The Astrophysical Journal

Abstract

The dielectric functions for graphite and astronomical silicate material are computed using available laboratory and astronomical data. It is noted that the magnetic dipole contribution to absorption in the infrared wavelengths can be important for conducting particles such as graphite. Formulas are given for evaluating electric and magnetic dipole cross-sections for small particles. Absorption cross-sections are evaluated for graphite and silicate particles with sizes between 0.003 and 1.0 microns, and wavelengths from 300 A to 1000 microns. On the basis of polarization profiles computed for both prolate and oblate graphite-silicate spheroids, it is concluded that interstellar silicate grain are predominantly oblate. Extinction curves are calculated for Mathis-Rumpl-Nordsieck graphite-silicate grain mixtures and are compared to observations. The model is found to be in good agreement with available infrared observations.

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Metadata

Authors
Draine, B. T., & Lee, H. M.
Venue
The Astrophysical Journal
Published
1984-10
Volume
285
Pages
89
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2006869439
Cited by
3,279
References
0
FWCI
31.28
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Optical properties of interstellar graphite and silicate grains. https://app.cochat.ai/papers/10.1086/162480
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Draine, B. T., & Lee, H. M. (1984). Optical properties of interstellar graphite and silicate grains. The Astrophysical Journal. https://doi.org/10.1086/162480

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