An Understanding of the Non-Thermal Radiation from the Crab Nebula

Details An Understanding of the Non-Thermal Radiation from the Crab Nebula An Understanding of the Non-Thermal Radiation from the Crab Nebula

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2385s&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The Crab nebula is the most extensively studied supernova remnant, which is powered by its pulsar. The remnant radation is non-thermal in nature measured over 20 decades in energy from radio to highenergy gamma rays. The propagation of electrons in the remnant has been studied in detail and the elecrons in the present epoch could explain the observed radiation over the entire energ domain. It is found that there are two kinds of accelerated spectrum that are required and we discuss some the conseqences.

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