The DOI matches its Crossref record; 179 of the 179 references it cites were found in a registry or an index.
The Dust Opacity of Star‐forming Galaxies
Open accessAbstract
Presence of dust in galaxies removes half or more of the stellar energy from the UV-optical budget of the Universe and has profound impact on our understanding of how galaxies evolve. Measures of opacity in local galaxies are reviewed together with widely used theoretical and empirical methods for quantifying its effects. Existing evidence shows that the dust content of nearby galaxies depends not only on their morphology, but also on their luminosity and activity level. A digression is devoted to starbursts in view of their potential relevance for measures of opacity in distant galaxies. Scarcity of coherent multiwavelength datasets hampers our ability to derive reliable obscuration estimates in intermediate and high redshift galaxies. This, in turn, limits the reliability of inferred physical quantities, such as star formation rates, stellar population ages, galaxy luminosity functions, and others.
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Cites
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Cited by
Draine, B. T. (2003) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.41.011802.094840 · Cited by 2,389
Modeling the Panchromatic Spectral Energy Distributions of Galaxies
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Self-citationDusty star-forming galaxies at high redshift
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THE SINS SURVEY OF z∼ 2 GALAXY KINEMATICS: PROPERTIES OF THE GIANT STAR-FORMING CLUMPS
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Metadata
- Authors
- Calzetti, D.
- Venue
- Publications of the Astronomical Society of the Pacific
- Publisher
- IOP Publishing
- Published
- 2001-12
- Volume
- 113
- Issue
- 790
- Pages
- 1449-1485
- ISSN
- 0004-6280 (ISSN-L)
- 1538-3873
- OpenAlex
- W1992881800
- Cited by
- 829
- References
- 179
- FWCI
- 15.07
- Type
- journal article
- Language
- en
- Open access
- green
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