Frequency Dependence of Radio Images of Supernova Remnants

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dc.creatorKarnaushenko, A. V.
dc.creatorBannikova, E. Yu.
dc.creatorKontorovich, V. M.
dc.date2007-12-10
dc.date.accessioned2026-07-07T08:48:17Z
dc.date.available2026-07-07T08:48:17Z
dc.descriptionRadio images of supernova remnants in the framework of diffusion model are discussed. The distribution profiles of synchrotron radiation intensity for spherical injection source of relativistic electrons are reduced at different frequencies. An explanation of the observational data obtained on UTR-2, according to which the size of the supernova remnant at decametric waves is larger than the remnant size at high frequencies, is given.
dc.descriptionPublished in Proceedings of the 14th Young Scientists Conference on Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007
dc.identifierhttps://arxiv.org/abs/0712.1484
dc.identifierhttp://arxiv.org/abs/0712.1484
dc.identifierYSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A. Golovin), Kyiv, Kyivskyi Universytet, pp. 36-39, 2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143893
dc.subjectAstrophysics
dc.titleFrequency Dependence of Radio Images of Supernova Remnants
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