Does CO trace H2 at high galactic latitude?

Computer Science

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Galaxy: Carbon Monoxide, Galaxy: Molecular Hydrogen, Molecular Clouds: Infrared Excesses

Scientific paper

The authors have recently completed a CO survey of 342 Infrared Excess Clouds (IRECs) distributed uniformly across the sky. Following comparison of the integrated CO brightness Wco (K km s-1) with the 100 μm infrared brightness B4 obtained from the IRAS data, they have found evidence for a threshold in B4 of 4 - 5 MJy sr-1 below which CO does not form.

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