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Fermi LAT Observation of Diffuse Gamma Rays Produced Through Interactions Between Local Interstellar Matter and High-energy Cosmic Rays
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2009 (English)In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 703, no 2, 1249-1256 p.Article in journal (Refereed) Published
Abstract [en]

Observations by the Large Area Telescope (LAT) on the Fermi mission of diffuse γ-rays in a mid-latitude region in the third quadrant (Galactic longitude l from 200° to 260° and latitude |b| from 22° to 60°) are reported. The region contains no known large molecular cloud and most of the atomic hydrogen is within 1 kpc of the solar system. The contributions of γ-ray point sources and inverse Compton scattering are estimated and subtracted. The residual γ-ray intensity exhibits a linear correlation with the atomic gas column density in energy from 100 MeV to 10 GeV. The measured integrated γ-ray emissivity is (1.63 ± 0.05) × 10-26 photons s-1sr-1 H-atom-1 and (0.66 ± 0.02) × 10-26 photons s-1sr-1 H-atom-1 above 100 MeV and above 300 MeV, respectively, with an additional systematic error of ~10%. The differential emissivity from 100 MeV to 10 GeV agrees with calculations based on cosmic ray spectra consistent with those directly measured, at the 10% level. The results obtained indicate that cosmic ray nuclei spectra within 1 kpc from the solar system in regions studied are close to the local interstellar spectra inferred from direct measurements at the Earth within ~10%.

Place, publisher, year, edition, pages
2009. Vol. 703, no 2, 1249-1256 p.
Keyword [en]
cosmic rays, diffuse radiation, gamma rays: observations
Identifiers
URN: urn:nbn:se:su:diva-33751DOI: 10.1088/0004-637X/703/2/1249ISI: 000269929500007ISBN: 0004-637X (print)OAI: oai:DiVA.org:su-33751DiVA: diva2:283830
Available from: 2009-12-30 Created: 2009-12-28 Last updated: 2017-12-12Bibliographically approved

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