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Cited by 2,389

The DOI matches its Crossref record; 89 of the 89 references it cites were found in a registry or an index.

Interstellar Dust Grains

Open access
Draine, B.T.·2003·Annual Review of Astronomy and Astrophysics

Abstract

▪ Abstract This review surveys the observed properties of interstellar dust grains: the wavelength-dependent extinction of starlight, including absorption features, from UV to infrared; optical luminescence; infrared emission; microwave emission; optical, UV, and X-ray scattering by dust; and polarization of starlight and of infrared emission. The relationship between presolar grains in meteorites and the interstellar grain population is discussed. Candidate grain materials and abundance constraints are considered. A dust model consisting of amorphous silicate grains, graphite grains, and polycyclic aromatic hydrocarbons is compared with observed emission and scattering. Some issues concerning evolution of interstellar dust are discussed.

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Crossref · 10.1146/annurev.astro.41.011802.094840

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Metadata

Authors
Draine, B. T.
Venue
Annual Review of Astronomy and Astrophysics
Published
2003-09
Volume
41
Issue
1
Pages
241-289
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2169198867
Cited by
2,389
References
89
FWCI
5.55
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Interstellar Dust Grains. https://app.cochat.ai/papers/10.1146/annurev.astro.41.011802.094840
The paper
Draine, B. T. (2003). Interstellar Dust Grains. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.41.011802.094840

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.