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- W3124137816 abstract "We report observations and analysis of infrared spectra of H3+ and CO lines in the Galactic center, within a few parsecs of the central black hole, Sgr A*. We find a cosmic ray ionization rate typically an order of magnitude higher than outside the Galactic center. Notwithstanding, the elevated cosmic ray ionization rate is 4 orders of magnitude too short to match the proton energy spectrum, as inferred from the recent discovery of the TeV γ-ray source in the vicinity of Sgr A*." @default.
- W3124137816 created "2021-02-01" @default.
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- W3124137816 date "2013-05-28" @default.
- W3124137816 modified "2023-10-17" @default.
- W3124137816 title "H<sub>3</sub><sup>+</sup> Spectroscopy and the Ionization Rate of Molecular Hydrogen in the Central Few Parsecs of the Galaxy" @default.
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- W3124137816 doi "https://doi.org/10.1021/jp400017s" @default.
- W3124137816 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/23617764" @default.
- W3124137816 hasPublicationYear "2013" @default.
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