The DOI matches its Crossref record; 28 of the 28 references it cites were found in a registry or an index.
GLOBAL COSMIC-RAY-RELATED LUMINOSITY AND ENERGY BUDGET OF THE MILKY WAY
Open accessAbstract
We use the GALPROP code for cosmic-ray (CR) propagation to calculate the broadband luminosity spectrum of the Milky Way related to CR propagation and interactions in the interstellar medium. This includes γ-ray emission from the production and subsequent decay of neutral pions (π 0 ), bremsstrahlung, and inverse Compton scattering, and synchrotron radiation. The Galaxy is found to be nearly a CR electron calorimeter, but only if γ-ray emitting processes are taken into account. Synchrotron radiation alone accounts for only one-third of the total electron energy losses with ∼10%–20% of the total synchrotron emission from secondary CR electrons and positrons. The relationship between far-infrared and radio luminosity that we find from our models is consistent with that found for galaxies in general. The results will be useful for understanding the connection between diffuse emissions from radio through γ-rays in "normal" (non-active galactic nucleus dominated) galaxies as well as for estimating the broadband extragalactic diffuse background from these kinds of galaxies.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Cosmic-Ray Propagation and Interactions in the Galaxy
Strong, A. W., Moskalenko, I. V., & Ptuskin, V. S. (2007) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev.nucl.57.090506.123011 · Cited by 1,161
Self-citationPropagation of Cosmic‐Ray Nucleons in the Galaxy
Strong, A. W., & Moskalenko, I. V. (1998) · The Astrophysical Journal · doi:10.1086/306470 · Cited by 1,051
Self-citationThe interstellar environment of our galaxy
Ferrière, K. M. (2001) · Reviews of Modern Physics · doi:10.1103/revmodphys.73.1031 · Cited by 1,019
Thermal infrared and nonthermal radio - Remarkable correlation in disks of galaxies
Helou, G., Soifer, B. T., & Rowan-Robinson, M. (1985) · The Astrophysical Journal · doi:10.1086/184556 · Cited by 942
Radio Properties of Infrared‐Selected Galaxies in the IRAS 2 Jy Sample
Yun, M. S., Reddy, N. A., & Condon, J. J. (2001) · The Astrophysical Journal · doi:10.1086/323145 · Cited by 928
Measurement of the Cosmic Raye++e−Spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope
Abdo, A. A., Ackermann, M., Ajello, M., Atwood, W. B., Axelsson, M., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., Battelino, M., et al. (2009) · Physical Review Letters · doi:10.1103/physrevlett.102.181101 · Cited by 904
Self-citationRadioactive 26Al from massive stars in the Galaxy
Diehl, R., Halloin, H., Kretschmer, K., Lichti, G. G., Schönfelder, V., Strong, A. W., von Kienlin, A., Wang, W., Jean, P., Knödlseder, J., et al. (2006) · Nature · doi:10.1038/nature04364 · Cited by 767
Self-citationProduction and Propagation of Cosmic‐Ray Positrons and Electrons
Moskalenko, I. V., & Strong, A. W. (1998) · The Astrophysical Journal · doi:10.1086/305152 · Cited by 766
Self-citationDiffuse Continuum Gamma Rays from the Galaxy
Strong, A. W., Moskalenko, I. V., & Reimer, O. (2000) · The Astrophysical Journal · doi:10.1086/309038 · Cited by 638
Self-citationStrong, A. W., Moskalenko, I. V., & Reimer, O. (2004) · The Astrophysical Journal · doi:10.1086/423193 · Cited by 514
Self-citation
Cited by
GIANT GAMMA-RAY BUBBLES FROM FERMI-LAT: ACTIVE GALACTIC NUCLEUS ACTIVITY OR BIPOLAR GALACTIC WIND?
Su, M., Slatyer, T. R., & Finkbeiner, D. P. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/724/2/1044 · Cited by 1,038
GeV OBSERVATIONS OF STAR-FORMING GALAXIES WITH THE FERMI LARGE AREA TELESCOPE
Ackermann, M., Ajello, M., Allafort, A., Baldini, L., Ballet, J., Bastieri, D., Bechtol, K., Bellazzini, R., Berenji, B., Bloom, E. D., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/755/2/164 · Cited by 391
Self-citationCONSTRAINTS ON COSMIC-RAY PROPAGATION MODELS FROM A GLOBAL BAYESIAN ANALYSIS
Trotta, R., Jóhannesson, G., Moskalenko, I. V., Porter, T. A., Ruiz de Austri, R., & Strong, A. W. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/729/2/106 · Cited by 332
Self-citationThe Nine Lives of Cosmic Rays in Galaxies
Grenier, I. A., Black, J. H., & Strong, A. W. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122457 · Cited by 320
Self-citationTHE FIRST FERMI LAT SUPERNOVA REMNANT CATALOG
Acero, F., Ackermann, M., Ajello, M., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., Bellazzini, R., Bissaldi, E., Blandford, R. D., et al. (2016) · The Astrophysical Journal Supplement Series · doi:10.3847/0067-0049/224/1/8 · Cited by 265
Self-citation
Metadata
- Authors
- Strong, A. W., Porter, T. A., Digel, S. W., Jóhannesson, G., Martin, P., Moskalenko, I. V., Murphy, E. J., & Orlando, E.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2010-09-20
- Volume
- 722
- Issue
- 1
- Pages
- L58-L63
- ISSN
- 2041-8205 (ISSN-L)
- 2041-8213
- OpenAlex
- W2034483141
- Cited by
- 268
- References
- 28
- FWCI
- 11.79
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: GLOBAL COSMIC-RAY-RELATED LUMINOSITY AND ENERGY BUDGET OF THE MILKY WAY. https://app.cochat.ai/papers/10.1088/2041-8205/722/1/l58
- The paper
- Strong, A. W., Porter, T. A., Digel, S. W., Jóhannesson, G., Martin, P., Moskalenko, I. V., Murphy, E. J., & Orlando, E. (2010). GLOBAL COSMIC-RAY-RELATED LUMINOSITY AND ENERGY BUDGET OF THE MILKY WAY. The Astrophysical Journal. https://doi.org/10.1088/2041-8205/722/1/l58
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
