Non-thermal emission from relativistic MHD simulations of pulsar wind nebulae: from synchrotron to inverse Compton

DOI10.1051/0004-6361:200809424zbMath1148.85323arXiv0804.1323OpenAlexW2596203452WikidataQ63411156 ScholiaQ63411156MaRDI QIDQ3519250

Elena Amato, D. Volpi, L. Del Zanna, N. Bucciantini

Publication date: 14 August 2008

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0804.1323

zbMATH Keywords

relativity magnetohydrodynamics (MHD)stars: pulsars: general ISM: supernova remnants radiation mechanisms: non-thermal ISM: individual objects: Crab Nebula

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

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