Cannon, John MWalter, FabianArmus, LeeBendo, George JCalzetti, DanielaDraine, Bruce TEngelbracht, Charles WHelou, GeorgeKennicutt, R CLeitherer, ClausRoussel, HeleneBot, CarolineBuckalew, Brent ADale, Daniel Ade Blok, WillemGordon, Karl DHollenbach, David J.Jarrett, Thomas HMeyer, M JMurphy, Eric JSheth, KartikThornley, Michele D2015-12-070004-637Xhttp://hdl.handle.net/1885/19691We present Spitzer imaging of the metal-deficient (Z ≃ 30% Z ⊙) Local Group dwarf galaxy NGC 6822. On spatial scales of ∼ 130 pc, we study the nature of IR, Hα, H I, and radio continuum emission. Nebular emission strength correlates with IR surfaceKeywords: Galaxies: dwarf; Galaxies: individual (NGC 6822); Galaxies: irregular; Galaxies: ISM; Infrared: galaxiesThe Nature of Infrared Emission in the Local Group Dwarf Galaxy NGC 6822 as Revealed by Spitzer200610.1086/5083412015-12-07