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• W2804208081 abstract "Gamma-ray observations of nearby radio-line-emitting gas structures in the interstellar medium allow us to probe the spectrum of cosmic rays (CRs). In this paper, we analysed Fermi Large Area Telescope (LAT) gamma-ray observations of three such structures located near each other to check if their CR spectra are compatible with that of the CR background or might provide evidence for a population of fresh CRs. We found that the shape of the gamma-ray spectrum in the Aquarius HI shell is consistent with the previously published stacked gamma-ray spectrum of the Gould Belt molecular clouds. We also found that assumptions on the diffuse Galactic gamma-ray background affect the spectral shapes of CRs derived in the R Coronae Australis and rho Ophiuchi molecular clouds in which spectral deviations had previously been suggested. These two facts provide evidence to support the hypothesis of uniformity of the shapes of cosmic ray spectra in the local Galaxy environment." @default.
• W2804208081 created "2018-06-01" @default.
• W2804208081 creator A5047793211 @default.
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• W2804208081 date "2018-05-14" @default.
• W2804208081 modified "2023-10-14" @default.
• W2804208081 title "Testing spatial uniformity of the CR spectrum in the local ISM with γ-ray observations" @default.
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• W2804208081 doi "https://doi.org/10.1093/mnras/sty1234" @default.
• W2804208081 hasPublicationYear "2018" @default.
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