The CO-to-H2 conversion factor of molecular outflows. Rovibrational CO emission in NGC 3256-S resolved by JWST/NIRSpec (2023)

First Author: Pereira-Santaella M
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