<i>Planck</i>early results. XVII. Origin of the submillimetre excess dust emission in the Magellanic Clouds
<i>Planck</i>early results. XVII. Origin of the submillimetre excess dust emission in the Magellanic Clouds
The integrated Spectral Energy Distributions of the Large and Small Magellanic Cloud appear significantly flatter than expected from dust models based on their FIR and radio emission. The origin of this millimetre excess is still unexplained, and is here investigated using the Planck data. The background CMB contribution is subtracted …