On the kinematics of a corotating relativistic plasma stream in the perpendicular rotator model of a pulsar magnetosphere

DOI10.1007/BF00653766zbMath0900.76791arXivastro-ph/9711265WikidataQ63390545 ScholiaQ63390545MaRDI QIDQ1368987

T. A. Kahniashvili, I. S. Nanobashvili, G. Z. Machabeli, O. V. Chedia

Publication date: 9 September 1998

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/9711265

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (2)

Spin-rotation couplings: spinning test particles and Dirac field ⋮ PARTICLE ACCELERATION CLOSE TO THE SUPERMASSIVE BLACK HOLE HORIZON: THE CASE OF M87

Cites Work

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• The global structure of the pulsar magnetospheres
• Relativistic magnetohydrodynamic winds of finite temperature

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