{ "id": "1902.09654", "version": "v1", "published": "2019-02-25T23:08:56.000Z", "updated": "2019-02-25T23:08:56.000Z", "title": "Interpreting the relation between the gamma-ray and infrared luminosities of star-forming galaxies", "authors": [ "Yi Zhang", "Fang-Kun Peng", "Xiang-Yu Wang" ], "comment": "9 pages, 4 figures, Accepted by ApJ", "categories": [ "astro-ph.HE", "astro-ph.GA" ], "abstract": "It has been found that there is a quasi-linear scaling relationship between the gamma-ray luminosity in GeV energies and the total infrared luminosity of star-forming galaxies, i.e. $L_{\\gamma}\\propto L_{\\rm IR}^{\\alpha}$ with $\\alpha\\simeq 1$. However, the origin of this linear slope is not well understood. Although extreme starburst galaxies can be regarded as calorimeters for hadronic cosmic ray interaction and thus a quasi-linear scaling may hold, it may not be the case for low star-formation-rate (SFR) galaxies, as the majority of cosmic rays in these galaxies are expected to escape. We calculate the gamma-ray production efficiency in star-forming galaxies by considering realistic galaxy properties, such as the gas density and galactic wind velocity in star-forming galaxies. We find that the slope for the relation between gamma-ray luminosity and the infrared luminosity gets steeper for low infrared luminosity galaxies, i.e. $\\alpha\\rightarrow 1.6$, due to increasingly lower efficiency for the production of gamma-ray emission. We further find that the measured data of the gamma-ray luminosity is compatible with such a steepening. The steepening in the slope suggests that cosmic-ray escape is very important in low-SFR galaxies.", "revisions": [ { "version": "v1", "updated": "2019-02-25T23:08:56.000Z" } ], "analyses": { "keywords": [ "star-forming galaxies", "gamma-ray luminosity", "hadronic cosmic ray interaction", "galactic wind velocity", "low infrared luminosity galaxies" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }