Why do the microstructures of the main pulse and the interpulse of the pulsar in the Crab nebula differ so dramatically?

DOI10.1134/S0040577920030113zbMath1444.85003OpenAlexW3015613359MaRDI QIDQ2193700

V. M. Kontorovich

Publication date: 20 August 2020

Published in: Theoretical and Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0040577920030113

zbMATH Keywords

pulsarneutron starCrab nebula pulsarinterpulsemain pulsepulse microstructureradiation mechanism

Mathematics Subject Classification ID

Strong interaction, including quantum chromodynamics (81V05) Galactic and stellar structure (85A15) Radiative transfer in astronomy and astrophysics (85A25)

Cites Work

• MHD Flows in Compact Astrophysical Objects
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