We investigate dust attenuation and its dependence on viewing angle for 308 star-forming galaxies at 1.3 ≤
This content will become publicly available on September 1, 2025
Dust is a key component of galaxies, but its properties during the earliest eras of structure formation remain elusive. Here we present a simple semi-analytic model of the dust distribution in galaxies at
- Award ID(s):
- 2205900
- PAR ID:
- 10550061
- Publisher / Repository:
- Journal of Cosmology and Astroparticle Physics
- Date Published:
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Volume:
- 2024
- Issue:
- 09
- ISSN:
- 1475-7516
- Page Range / eLocation ID:
- 018
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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