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Title: Fermi large area telescope discovery of GeV gamma-ray emission from the vicinity of SNR W44

Journal Article · · The Astrophysical Journal. Letters
 [1];  [1];  [2];  [3];  [4];  [5];  [6];  [7]
  1. SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
  2. Ibaraki Univ., Mito (Japan)
  3. SLAC National Accelerator Lab., Menlo Park, CA (United States)
  4. Univ. of Bordeaux (France). Gradignan Bordeaux Nucearl Research Center
  5. Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; Nagoya Univ. (Japan). Solar-Terrestrial Environment Lab.
  6. Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
  7. Inst. of Sciences in Spain and Catalan Institution for Research and Advanced Studies (ICREA), Barcelona (Spain)

Here, we report the detection of GeV γ-ray emission from the molecular cloud complex that surrounds the supernova remnant (SNR) W44 using the Large Area Telescope on board Fermi. And while the previously reported γ-ray emission from SNR W44 is likely to arise from the dense radio-emitting filaments within the remnant, the γ-ray emission that appears to come from the surrounding molecular cloud complex can be ascribed to the cosmic rays (CRs) that have escaped from W44. Furthermore, the non-detection of synchrotron radio emission associated with the molecular cloud complex suggests the decay of π0 mesons produced in hadronic collisions as the γ-ray emission mechanism. The total kinetic energy channeled into the escaping CRs is estimated to be W esc ~ (0.3-3) × 1050 erg, in broad agreement with the conjecture that SNRs are the main sources of Galactic CRs.

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:
1356744
Journal Information:
The Astrophysical Journal. Letters, Vol. 749, Issue 2; ISSN 2041-8205
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 68 works
Citation information provided by
Web of Science

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Cited By (20)

The e-ASTROGAM mission: Exploring the extreme Universe with gamma rays in the MeV – GeV range journal June 2017
The supernova remnant W44: Confirmations and challenges for cosmic-ray acceleration journal May 2014
Cosmic-ray propagation in the bi-stable interstellar medium: I. Conditions for cosmic-ray trapping journal February 2019
THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS journal September 2013
Anisotropic cosmic ray diffusion and gamma-ray production close to supernova remnants, with an application to W28 journal December 2012
A Chandra X-ray study of the mixed-morphology supernova remnant 3C 400.2 journal December 2014
Non-linear diffusion of cosmic rays escaping from supernova remnants – I. The effect of neutrals journal July 2016
Investigating the high-frequency spectral features of SNRs Tycho, W44, and IC443 with the Sardinia Radio Telescope journal May 2018
Towards observing reverberating and superefficient pulsar wind nebulae journal March 2019
Detection of the Characteristic Pion-Decay Signature in Supernova Remnants journal February 2013
The Important Role of Cosmic-Ray Re-Acceleration journal April 2019
Discovery of Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Kesteven 79 journal September 2018
The Second Fermi Large area Telescope Catalog of Gamma-Ray Pulsars text January 2013
Detection of the Characteristic Pion-Decay Signature in Supernova Remnants text January 2013
The e-ASTROGAM mission text January 2017
Analytic Solution for Self-regulated Collective Escape of Cosmic Rays from their Acceleration Sites text January 2012
Non-linear diffusion of cosmic rays escaping from supernova remnants - I. The effect of neutrals text January 2016
The e-ASTROGAM mission (exploring the extreme Universe with gamma rays in the MeV-GeV range) text January 2016
Discovery of molecular and atomic clouds associated with the gamma-ray supernova remnant Kesteven 79 text January 2017
Towards observing reverberating and superefficient pulsar wind nebulae text January 2019