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Post Info TOPIC: Perseus Molecular Cloud


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Perseus Molecular Cloud
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The Perseus molecular cloud is a nearby (600 ly) Giant Molecular Cloud in the constellation of Perseus and contains over 10,000 solar masses of gas and dust covering an area of 6 by 2 degrees.
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Title: AMI Observations of the Anomalous Microwave Emission in the Perseus Molecular Cloud
Authors: C. T. Tibbs, A. M. M. Scaife, C. Dickinson, R. Paladini, R. D. Davies, R. J. Davis, K. J. B. Grainge, R. A. Watson

We present observations of the known anomalous microwave emission region, G159.6-18.5, in the Perseus molecular cloud at 16 GHz performed with the Arcminute Microkelvin Imager Small Array. These are the highest angular resolution observations of G159.6-18.5 at microwave wavelengths. By combining these microwave data with infrared observations between 5.8 and 160 µm from the Spitzer Space Telescope, we investigate the existence of a microwave - infrared correlation on angular scales of ~2 arcmin. We find that the overall correlation appears to increase towards shorter infrared wavelengths, which is consistent with the microwave emission being produced by electric dipole radiation from small, spinning dust grains. We also find that the microwave - infrared correlation peaks at 24 µm (6.7\sigma), suggesting that the microwave emission is originating from a population of stochastically heated small interstellar dust grains rather than polycyclic aromatic hydrocarbons.

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