A New Radio Emission Mechanism in the ISM

Details A New Radio Emission Mechanism in the ISM A New Radio Emission Mechanism in the ISM

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..344..140c&link_type=abstract

The Cool Universe: Observing Cosmic Dawn, ASP Conference Series, Vol. 344, Proceedings of the conference held 4-8 October, 2004

Astronomy and Astrophysics

Astronomy

1

Scientific paper

A byproduct of experiments designed to map the CMB is the recent detection of a new component of foreground Galactic emission. The anomalous foreground at 10--30 GHz, unexplained by traditional emission mechanisms, correlates with 100 micron dust emission, and is thus presumably due to dust.
Is the anomalous foreground ubiquitous in the Galaxy? We present evidence obtained with the CBI experiment supporting the existence of the new component in specific objects, in the form of a 31 GHz excess over free-free emission in H II regions, planetary nebulae, and a surprisingly radio-bright dark cloud.

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