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Characterising anomalous microwave emission from spinning dust

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I will review the current observational evidence for spinning dust emission with an emphasis on targeted measurements towards galactic objects. These data are often contradictory and a number of alternative physical processes must be dismissed before many detections in the literature can be verified as definitively arising from spinning dust. I will discuss the limitations of currently available datasets and the potential for future work on this subject.

This talk is part of the Cavendish Astrophysics Seminars series.

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