BIANCHI, SimoneSimoneBIANCHI2023-01-252023-01-2520201743-9213http://hdl.handle.net/20.500.12386/33060Far-infrared photometric observations from the Herschel Space Observatory offer the opportunity to study the dust-to-gas ratio at a resolved scale in nearby galaxies. The amount, and gradient, of solid-phase metals can thus be compared with metallicity measurements in the gas phase. We describe our preliminary work on the topic with data from the DustPedia project.ELETTRONICOenConference paper10.1017/S17439213190042042-s2.0-85080919832https://api.elsevier.com/content/abstract/scopus_id/85080919832https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/dusttogas-ratio-and-metallicity-gradients-in-dustpedia-galaxies/F3220CF5122249CD0DDDDFA6AF44AF2C2020IAUGA..30..251BFIS/05 - ASTRONOMIA E ASTROFISICA