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Title: Fermi LAT Observation of Diffuse Gamma Rays Produced Through Interactions Between Local Interstellar Matter and High-Energy Cosmic Rays

Journal Article · · The Astrophysical Journal
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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 in this paper. 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. Finally, 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%.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
Fermi LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1357436
Journal Information:
The Astrophysical Journal, Vol. 703, Issue 2; ISSN 0004-637X
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 94 works
Citation information provided by
Web of Science

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Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud: II. 30 Doradus journal August 2019
THE DIFFUSE GAMMA-RAY BACKGROUND FROM TYPE Ia SUPERNOVAE journal February 2012
Global Cosmic-Ray-Related Luminosity and Energy Budget of the Milky way journal September 2010
Possible GeV counterpart at the ground level associated with Fermi LAT gamma-ray bursts journal July 2018
Dark matter relic abundance and big bang nucleosynthesis in Horava’s gravity journal May 2011
Diffuse Galactic Gamma Rays from Shock-Accelerated Cosmic Rays journal August 2012
A Cocoon of Freshly Accelerated Cosmic Rays Detected by Fermi in the Cygnus Superbubble journal November 2011
Neutrino Coupling to Cosmological Background: a Review on Gravitational Baryo/Leptogenesis journal October 2013
Evidence for Cosmic-Ray Escape in the Small Magellanic Cloud Using Fermi Gamma Rays journal October 2018
Possible Detection of Gamma-Rays from Epsilon Eridani journal June 2019
Fermi -LAT Observations of γ -Ray Emission toward the Outer Halo of M31 journal July 2019
Cosmic Rays in the Heliosphere: Requirements for Future Observations book January 2012
Fermi-LAT Observations of Gamma-Ray Emission Towards the Outer Halo of M31 conference July 2019
Constraints on cosmic-ray propagation models from a global Bayesian analysis text January 2010
The Diffuse Gamma-ray Background from Type Ia Supernovae text January 2012
Fermi-LAT Observations of the Diffuse Gamma-Ray Emission: Implications for Cosmic Rays and the Interstellar Medium text January 2012
Diffuse Galactic Gamma Rays from Shock-Accelerated Cosmic Rays text January 2012
Nonthermal X-rays from low-energy cosmic rays: Application to the 6.4 keV line emission from the Arches cluster region text January 2012
Evidence for Cosmic-Ray Escape in the Small Magellanic Cloud using Fermi Gamma-rays text January 2018
Possible GeV counterpart at the ground level associated with Fermi LAT gamma-ray bursts text January 2018