The role of grain size in active galactic nuclei torus dust models (2023)
Attributed to:
Astrophysics at Oxford 2019-2022
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202345858
Publication URI: http://dx.doi.org/10.1051/0004-6361/202345858
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics