2015ApJ...805...50A

We analyze the gamma ray emission from nine high latitude, translucent molecular clouds taken with the Fermi Large Area Telescope between 250 MeV and 10 GeV. Observations of gamma rays allow us to probe the density and spectrum of cosmic rays in the solar neighborhood. The clouds studied lie within ∼270 pc from the Sun and are selected from the Planck all-sky CO map. Gamma rays in this energy range mostly result from cosmic-ray interactions with the interstellar medium, which is traced with three components: H i, CO, and dark gas. Every cloud is detected and shows significant, extended gamma ray emission from molecular gas. The gamma ray emission is dominated by the CO-emitting gas in some clouds, but by the CO-dark gas in others. The average emissivity and gamma ray power law index from H i above 1 GeV shows no evidence of a systematic variation. The CO-to- conversion factor shows no variation between clouds over this small spatial range, but shows significant variations within each cloud. The average CO-to- conversion factor suggests that the CO-dark gas is molecular as opposed to optically thick H i.