Fermi LAT Study of the Cosmic-rays and the Interstellar Medium in Nearby Molecular Clouds
Katsuhiro Hayashi, Tsunefumi Mizuno, (on behalf of the Fermi-LAT, collaboration)

TL;DR
This study uses Fermi LAT gamma-ray data to analyze cosmic-ray densities and molecular gas properties in nearby molecular clouds, revealing variations in cosmic-ray density and molecular mass calibration ratios close to the solar system.
Contribution
First detailed gamma-ray analysis of multiple nearby molecular clouds to measure cosmic-ray densities and molecular gas properties near the solar system.
Findings
Cosmic-ray density varies by about 20% among the regions.
The molecular mass calibration ratio, X_CO, ranges from 0.6 to 1.0 x 10^{20} H2 molecules cm^{-2} (K km s^{-1})^{-1}.
Similar amounts of dark gas are inferred at atomic-molecular interfaces.
Abstract
We report an analysis of the interstellar gamma-ray emission from nearby molecular clouds Chamaeleon, R Coronae Australis (R CrA), and Cepheus and Polaris flare regions with the {\it Fermi} Large Area Telescope (LAT). They are among the nearest molecular cloud complexes, within 300 pc from the solar system. The gamma-ray emission produced by interactions of cosmic-rays (CRs) and interstellar gas in those molecular clouds is useful to study the CR densities and distributions of molecular gas close to the solar system. The obtained gamma-ray emissivities from 250 MeV to 10 GeV for the three regions are about (6--10) 10 photons s sr H-atom, indicating a variation of the CR density by 20% even if we consider the systematic uncertainties. The molecular mass calibration ratio, , is found to be about…
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