Hostname: page-component-788cddb947-55tpx Total loading time: 0 Render date: 2024-10-19T20:49:23.746Z Has data issue: false hasContentIssue false
  • English
  • Français

About the Magnetic Field Generation in Crab Nebula

Published online by Cambridge University Press:  12 April 2016

Irakli S. Nanobashvili
Irakli S. Nanobashvili*
Affiliation:
Abastumani Astrophysical Observatory, Georgian Academy of Sciences, A. Kazbegi Ave.2a, GE-380060 Tbilisi, Georgia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The new plasma mechanism for the magnetic field generation in Crab Nebula is suggested. The mechanism is based on the development of two-stream instability after the supernova explosion.

Type
Part 9. Population and Neutron Star Properties
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 609 - 610
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Shklovsky, I.S. 1953, DAN SSSR, 90, 983. (in Russian)Google Scholar
Vashakidze, M.A. 1954, Astron. Circ., No 147. (in Russian)Google Scholar
Piddington, N.S. 1957, Australian J. Phys., 10, 350.Google Scholar
Kennel, C.F. & Coroniti, F.V. 1984, ApJ, 283, 694.Google Scholar
Kennel, C.F. & Coroniti, F.V. 1984, ApJ, 710, 694.Google Scholar
Tsikarishvili, E.G., Chagelishvili, G.D., Chedia, O.V., Lominadze, J.G & Sokhadze, Z.A. 1988, Ap&SS, 149, 255.Google Scholar
Machabeli, G.Z., Nanobashvili, I.S. & Tendier, M. 1999, Physica Scripta, accepted for publication.Google Scholar