A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data (2022)
Attributed to:
Astrophysics at Oxford 2019-2022
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2208.11620
Publication URI: https://arxiv.org/abs/2208.11620
Type: Other