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Effective shielding of ≲10 GeV cosmic rays from dense molecular clumps - Nature Astronomy

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Effective shielding of ≲10 GeV cosmic rays from dense molecular clumps - Nature Astronomy

The density of cosmic rays inside molecular clouds determines the ionization rate in the dense cores where stars form. It is also one of the drivers of astrochemistry leading to the creation of complex molecules. Through Fermi Large Area Telescope observations of nearby giant molecular clouds, we observed deficits (holes) in the gamma-ray residual map when modelling with the expected gamma-ray diffuse emission from uniform cosmic rays interacting with the molecular content.

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Effective shielding of ≲10 GeV cosmic rays from dense molecular clumps - Nature Astronomy

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Effective shielding of ≲10 GeV cosmic rays from dense molecular clumps - Nature Astronomy

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