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The Kinematics of Polycyclic Aromatic Hydrocarbons (PAHs) in Galaxies revealed by Principal Component Analysis (PCA) tomography with JWST/NIRSpec (2024)

First Author: Donnan F

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.2405.13669

Publication URI: https://arxiv.org/abs/2405.13669

Type: Preprint