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Title: Local H i emissivity measured with FERMI-LAT and implications for Cosmic-ray spectra

Journal Article · · The Astrophysical Journal (Online)
 [1]
  1. CEA-IRFU/CNRS/Univ. Paris Diderot, Gif-sur-Yvette (France)

Cosmic-ray (CR) electrons and nuclei interact with the Galactic interstellar gas and produce high-energy γ-rays. The γ-ray emission rate per hydrogen atom, called emissivity, provides a unique indirect probe of the CR flux. We present the measurement and the interpretation of the emissivity in the solar neighborhood for γ-ray energy from 50 MeV to 50 GeV. We analyzed a subset of 4 yr of observations from the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope (Fermi) restricted to absolute latitudes $$10^\circ \lt | b| \lt 70^\circ $$. From a fit to the LAT data including atomic, molecular, and ionized hydrogen column density templates, as well as a dust optical depth map, we derived the emissivities, the molecular hydrogen–to–CO conversion factor $${X}_{\mathrm{CO}}=(0.902\pm 0.007)\times {10}^{20}$$ cm–2 (K km s–1)–1, and the dust-to-gas ratio $${X}_{\mathrm{DUST}}=(41.4\pm 0.3)\times {10}^{20}$$ cm–2 mag–1. Moreover, we detected for the first time γ-ray emission from ionized hydrogen. We compared the extracted emissivities to those calculated from γ-ray production cross sections and to CR spectra measured in the heliosphere. We observed that the experimental emissivities are reproduced only if the solar modulation is accounted for. This provides a direct detection of solar modulation observed previously through the anticorrelation between CR fluxes and solar activity. Lastly, we fitted a parameterized spectral form to the heliospheric CR observations and to the Fermi-LAT emissivity and obtained compatible local interstellar spectra for proton and helium kinetic energy per nucleon between between 1 and 100 GeV and for electron–positrons between 0.1 and 100 GeV.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1355151
Journal Information:
The Astrophysical Journal (Online), Vol. 806, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 42 works
Citation information provided by
Web of Science

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Cited By (17)

Galactic bulge preferred over dark matter for the Galactic centre gamma-ray excess journal March 2018
Cosmic rays, gas and dust in nearby anticentre clouds: I. CO-to-H journal May 2017
Exploring the shape of the γ -ray spectrum around the “ π 0 -bump” journal July 2018
Hard and bright gamma-ray emission at the base of the Fermi bubbles journal May 2019
The cosmic-ray content of the Orion-Eridanus superbubble journal March 2020
On the progressive hardening of the cosmic-ray proton spectrum in the inner Galaxy journal October 2018
Imprints of cosmic rays in multifrequency observations of the interstellar emission journal December 2017
Gamma-Ray Emission from Molecular Clouds Generated by Penetrating Cosmic Rays journal November 2018
Fermi -LAT Observations of γ -Ray Emission toward the Outer Halo of M31 journal July 2019
Fermi -LAT γ -Ray Study of the Interstellar Medium and Cosmic Rays in the Chamaeleon Molecular Cloud Complex: A Look at the Dark Gas as Optically Thick H i journal October 2019
Galactic bulge preferred over dark matter for the Galactic centre gamma-ray excess text January 2018
Fermi-LAT Observations of Gamma-Ray Emission Towards the Outer Halo of M31 conference July 2019
Galactic Bulge Preferred Over Dark Matter for the Galactic Center Gamma-Ray Excess text January 2016
Imprints of Cosmic Rays in Multifrequency Observations of the Interstellar Emission text January 2017
On the progressive hardening of the cosmic-ray proton spectrum in the inner Galaxy text January 2018
Hard and bright gamma-ray emission at the base of the Fermi bubbles text January 2019
The cosmic-ray content of the Orion-Eridanus superbubble text January 2020

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