Computer Science
Scientific paper
Apr 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xrrc.proce7.10b&link_type=abstract
"X-Ray and Radio Connections (eds. L.O. Sjouwerman and K.K Dyer) Published electronically by NRAO, http://www.aoc.nrao.edu/event
Computer Science
X-Ray, Radio, Dissipation Of Jets
Scientific paper
The similarity and difference between the images of jets of extragalactic sources in radio and X-ray bands, created by the same distribution of relativistic electrons due to synchrotron (for radio) and inverse Compton scattering (for X-ray) is discussed. We restrict ourselves to the vicinity of the moving sources of relativistic electrons --- jet knots and hot spots --- with diffusion as the spreading mechanism of the electrons. The case of independence on coordinates purely Compton losses on relic radiation is considered. The form of ``flares'' near jet knots is investigated. It is shown, that the heterogeneity of a magnetic field can result in characteristic differences in the form and location of radio and X-ray isophotes depending whether the magnetic field decreases or increases to the periphery of the source.
Bannikova Elena Yu.
Kontorovich Victor M.
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