A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data (2022)
Attributed to:
Astrophysics at Oxford 2022 -2025
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202244806
Publication URI: http://dx.doi.org/10.1051/0004-6361/202244806
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics