0.4–2 keV X-ray and SZ images of the Coma cluster. Compact sources have been excised from the X-ray image before smoothing with the broad Gaussian (σ = 200′′). The size of the smoothing kernel was chosen to approximately match the angular resolution of the Planck Y-map. Contours from SZ image are shown in both panels. Many non-axisymmetric features in these two images match suggesting that they are due to the presence of hot gas.