Sgr B2(DS) contains an H II region whose radio continuum mixes thermal free-free and extended non-thermal synchrotron emission, plausibly produced by first-order Fermi acceleration at the bubble edge.
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The physical and chemical structure of Sagittarius B2 -- V. Non-thermal emission in the envelope of Sgr B2
Sgr B2(DS) contains an H II region whose radio continuum mixes thermal free-free and extended non-thermal synchrotron emission, plausibly produced by first-order Fermi acceleration at the bubble edge.