{ "id": "2101.03732", "version": "v1", "published": "2021-01-11T07:32:47.000Z", "updated": "2021-01-11T07:32:47.000Z", "title": "Roll of Polycyclic Aromatic Hydrocarbons on the Cosmic-Ray ionization rate in the Galaxy", "authors": [ "Gargi Shaw", "G. J. Ferland" ], "comment": "Accepted for publication in ApJ, 31 pages, 22 figures", "categories": [ "astro-ph.GA" ], "abstract": "The cosmic-ray ionization rate ($\\zeta$, s$^{-1}$) plays an important role in the interstellar medium. It controls ion-molecular chemistry and provides a source of heating. Here we perform a grid of calculations using the spectral synthesis code CLOUDY along nine sightlines towards, HD 169454, HD 110432, HD 204827, $\\lambda$ Cep, X Per, HD 73882, HD 154368, Cyg OB2 5, Cyg OB2 12. The value of $\\zeta$ is determined by matching the observed column densities of H$_3^+$ and H$_2$. The presence of polycyclic aromatic hydrocarbons (PAHs) affects the free electron density, which changes the H$_3^+$ density and the derived ionization rate. PAHs are ubiquitous in the Galaxy, but there are also regions where PAHs do not exist. Hence, we consider clouds with a range of PAH abundances and show their effects on the H$_3^+$ abundance. We predict an average cosmic-ray ionization rate for H$_2$ ($\\zeta$(H$_2$))= (7.88 $\\pm$ 2.89) $\\times$ 10$^{-16}$ s$^{-1}$ for models with average Galactic PAHs abundances, (PAH/H =10$^{-6.52}$), except Cyg OB2 5 and Cyg OB2 12. The value of $\\zeta$ is nearly 1 dex smaller for sightlines toward Cyg OB2 12. We estimate the average value of $\\zeta$(H$_2$)= (95.69 $\\pm$ 46.56) $\\times$ 10$^{-16}$ s$^{-1}$ for models without PAHs.", "revisions": [ { "version": "v1", "updated": "2021-01-11T07:32:47.000Z" } ], "analyses": { "keywords": [ "polycyclic aromatic hydrocarbons", "cyg ob2", "spectral synthesis code cloudy", "average cosmic-ray ionization rate", "average galactic pahs abundances" ], "note": { "typesetting": "TeX", "pages": 31, "language": "en", "license": "arXiv", "status": "editable" } } }