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Polarization characteristics of the Crab pulsar’s giant radio pulses at HFCs phases

  • We discuss our recent discovery of the giant radio emission from the Crab pulsar at its high frequency components (HFCs) phases and show the polarization characteristic of these pulses. This leads us to a suggestion that there is no difference in the emission mechanism of the main pulse (MP), interpulse (IP) and HFCs. We briefly review the size distributions of the Crab giant radio pulses (GRPs) and discuss general characteristics of the GRP phenomenon in the Crab and other pulsars.

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Metadaten
Document Type:Conference Object
Language:English
Author:A. Słowikowska, A. Jessner, B. Klein, G. Kanbach
Parent Title (English):Bulik, Rudak et al. (Eds.): Astrophysical Sources of High Energy Particles and Radiation. Torun (Poland), 20-24 June 2005
First Page:324
Last Page:329
ISBN:0-7354-0290-6
DOI:https://doi.org/10.1063/1.2141893
Publisher:AIP Publishing
Date of first publication:2005/11/22
Keyword:Pulsars; electromagnetic wave polarisation; stellar radiation
Dewey Decimal Classification (DDC):5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften
Entry in this database:2015/10/09