CORDIS Project
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This project investigates unexpected radio emissions from dark interstellar clouds to understand their origins and implications for cosmic background studies. It aims to differentiate between two potential emission mechanisms: cold plasma radiation and spinning dust emission, which could reveal new insights into the in…
The anomalous foreground was detected 10 years ago as an unexpected Galactic screen at cm-wavelengths in experiments designed to map the Cosmic Microwave Background (CMB), seen in the direction of cirrus interstellar dust clouds and ubiquitous at high Galactic latitudes. A joint Universidad de Chile (U.
Ch.) and Caltech effort led to the discovery of surprisingly bright radio emission from canonical dark (i.e. dusty) clouds: rho Oph and M78, as well as translucent LDN1780 and zeta Oph.
What is t…
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