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  Origin of the very high energy gamma-ray emission from pulsar wind nebulae

Giacinti, G., Reville, B., & Kirk, J. (2021). Origin of the very high energy gamma-ray emission from pulsar wind nebulae. Proceedings of Science, 395: 913. doi:10.22323/1.395.0913.

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https://pos.sissa.it/395/913/pdf (Publisher version)
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 Creators:
Giacinti, G.1, Author           
Reville, B.1, Author           
Kirk, J.2, Author           
Affiliations:
1Brian Reville, Astrophysical Plasma Theory (APT) - Max Planck Research Group, Junior Research Groups, MPI for Nuclear Physics, Max Planck Society, ou_3055242              
2Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society, ou_2074298              

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 Dates: 2021-07
 Publication Status: Published online
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 Rev. Type: -
 Identifiers: DOI: 10.22323/1.395.0913
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Title: 37th International Cosmic Ray Conference (ICRC2021) - CRI - Cosmic Ray Indirect
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Title: Proceedings of Science
  Other : PoS
Source Genre: Journal
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Pages: - Volume / Issue: 395 Sequence Number: 913 Start / End Page: - Identifier: ISSN: 1824-8039
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000018850_1