{ "id": "2405.13669", "version": "v1", "published": "2024-05-22T14:09:33.000Z", "updated": "2024-05-22T14:09:33.000Z", "title": "The Kinematics of Polycyclic Aromatic Hydrocarbons (PAHs) in Galaxies revealed by Principal Component Analysis (PCA) tomography with JWST/NIRSpec", "authors": [ "Fergus R. Donnan", "Dimitra Rigopoulou", "Ismael GarcĂ­a-Bernete" ], "comment": "Accepted for publication in MNRAS Letters. Online supplementary material is included", "categories": [ "astro-ph.GA" ], "abstract": "Polycyclic Aromatic Hydrocarbons (PAHs) are organic molecules which comprise the smallest particles of dust in the interstellar medium (ISM). Due to their broad/complex emission profiles, obtaining kinematics is a challenge with traditional methods, especially before the advent of the JWST. In this work we employ Principal Component Analysis (PCA) tomography to analyse JWST/NIRSpec IFU data of 3 nearby luminous infrared galaxies (LIRGs), namely, NGC 3256 N, NGC 3256 S and NGC 7469. We detect the signature of rotation in the second principal component of the 3.3 $\\mu$m PAH feature in all three targets. We construct velocity maps from the principal components for the 3.3 $\\mu$m PAH feature, Br$\\beta$ (2.625$\\mu$m) and molecular hydrogen, H$_2$ 1-0 S(1) (2.12$\\mu$m). We find that in each target, the PAHs qualitatively follow the rotation of the galaxy, consistent with the rotational signature derived from Br$\\beta$ and H$_2$. There are however some differences, with the PAH rotation in NGC 3256 N appearing at a different position angle, which suggest differences in the motion of the dust as compared to the gas. This kind of analysis opens a new window into this key component of the ISM.", "revisions": [ { "version": "v1", "updated": "2024-05-22T14:09:33.000Z" } ], "analyses": { "keywords": [ "polycyclic aromatic hydrocarbons", "tomography", "kinematics", "analyse jwst/nirspec ifu data", "pah feature" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }