Detection of spectral variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
Anomalous Microwave Emission (AME) is a significant component of Galactic diffuse emission in the frequency range 10- $60\, \mathrm{GHz}$ and a new window into the properties of sub-nanometre-sized grains in the interstellar medium. We investigate the morphology of AME in the ≍10 ○ diameter λ Orionis ring by combining intensity data from the
Cepeda-Arroita, R. et al.
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2021