Abstract
The Herschel HIFI Key Program, G alactic O bservations of T erahertz C + ( GOT C+ ) is a survey of [CII] 1.9 THz emission throughout the Galaxy. Comparison of the first results of this survey with HI and CO isotopomer emission reveals excess [CII] emission beyond that expected from HI and CO layers alone, and is best explained as coming from a hidden layer of H 2 gas, the so-called ISM “dark gas”.
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