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Dominique M. -A. Meyer

3 papers here

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  • sole author1
  • last author1

Across the 2 of 3 papers where every author was matched, so the position is known.

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  • astro-ph.HE3

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most citedSensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

22 citations · 22 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2024

On the origin of mixed morphology supernova remnants: Linking their properties to the evolution of a red supergiant progenitor star

Alexandros Chiotellis, Emmanouil Zapartas, Dominique M. -A. Meyer

Mixed-morphology supernova remnants (MMSNRs) are characterized by a shell-like morphology in the radio and centrally-peaked thermal emission in the X-ray band. The nature of this p…

astro-ph.HE2024

Stellar wind bubbles of OB stars as Galactic cosmic-ray re-accelerators

Dominique M. -A. Meyer

Cosmic rays are highly energetic messengers propagating in magnetized plasma, which are, possibly but not exclusively, accelerated at astrophysical shocks. Amongst the variety of a…

astro-ph.HE2023★ 22 cited

Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

The Cherenkov Telescope Array Consortium, F. Acero, A. Acharyya +356

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadr…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.