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Inverse Compton Origin of the Hard X‐Ray and Soft Gamma‐Ray Emission from the Galactic Ridge

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Porter, Troy A., Moskalenko, Igor V., Strong, Andrew W., Orlando, Elena, Bouchet, L.·2008·The Astrophysical Journal

Abstract

A recent redetermination of the nonthermal component of the hard X-ray to soft γ-ray emission from the Galactic ridge, using the SPI instrument on the International Gamma-Ray Astrophysics Laboratory ( INTEGRAL ), is shown to be well reproduced as inverse Compton emission from the interstellar medium. Both cosmic-ray primary electrons and secondary electrons and positrons contribute to the emission. The prediction uses the GALPROP model and includes a new calculation of the interstellar radiation field. This may solve a long-standing mystery of the origin of this emission, and potentially opens a new window on Galactic cosmic rays.

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Metadata

Authors
Porter, T. A., Moskalenko, I. V., Strong, A. W., Orlando, E., & Bouchet, L.
Venue
The Astrophysical Journal
Published
2008-07-20
Volume
682
Issue
1
Pages
400-407
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2129746122
Cited by
245
References
0
FWCI
11.10
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Inverse Compton Origin of the Hard X‐Ray and Soft Gamma‐Ray Emission from the Galactic Ridge. https://app.cochat.ai/papers/10.1086/589615
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Porter, T. A., Moskalenko, I. V., Strong, A. W., Orlando, E., & Bouchet, L. (2008). Inverse Compton Origin of the Hard X‐Ray and Soft Gamma‐Ray Emission from the Galactic Ridge. The Astrophysical Journal. https://doi.org/10.1086/589615

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.