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  Supernova remnants in the very-high-energy gamma-ray domain: the role of the Cherenkov telescope array

Cristofari, P., Gabici, S., Humensky, T. B., Santander, M., Terrier, R., Parizot, E., et al. (2017). Supernova remnants in the very-high-energy gamma-ray domain: the role of the Cherenkov telescope array. Monthly Notices of the Royal Astronomical Society, 471(1), 201-209. doi:10.1093/mnras/stx1574.

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 Creators:
Cristofari, P.1, Author
Gabici, S.2, Author           
Humensky, T. B.1, Author
Santander, M.1, Author
Terrier, R.1, Author
Parizot, E.1, Author
Casanova, S.2, Author           
Affiliations:
1external, ou_persistent22              
2Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              

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 MPINP: Hochenergie-Astrophysik Theorie - Abteilung Hofmann
 Abstract: Supernova remnants are often presented as the most probable sources of Galactic cosmic rays. This idea is supported by the accumulation of evidence that particle acceleration is happening at supernova remnant shocks. Observations in the TeV range have especially contributed to increase the understanding of the mechanisms, but many aspects of the particle acceleration at supernova remnant shocks are still debated. The Cherenkov telescope array is expected to lead to the detection of many new supernova remnants in the TeV and multi-TeV range. In addition to the individual study of each, the study of these objects as a population can help constrain the parameters describing the acceleration of particles and increase our understanding of the mechanisms involved.

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 Dates: 2017
 Publication Status: Issued
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 Rev. Type: -
 Identifiers: DOI: 10.1093/mnras/stx1574
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Title: Monthly Notices of the Royal Astronomical Society
  Other : Mon. Not. R. Astron. Soc.
Source Genre: Journal
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Publ. Info: Oxford : Oxford University Press
Pages: - Volume / Issue: 471 (1) Sequence Number: - Start / End Page: 201 - 209 Identifier: ISSN: 1365-8711
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000024150