The CO-to-H2 conversion factor of molecular outflows. Rovibrational CO emission in NGC 3256-S resolved by JWST/NIRSpec (2023)
Attributed to:
Astrophysics at Oxford 2019-2022
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2309.06486
Publication URI: https://arxiv.org/abs/2309.06486
Type: Preprint