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Cygnus a and the Williams model,ndary’ hot spot in each lobe, as well as the jets which feed the primaries. We interpret our observations along the line of the Williams and Gull (1986) ‘splatter spot’ models for double hot spots is extragalactic radio sources.附录 发表于 2025-3-22 13:10:08
Multifrequency flux determination in the hot spot of 3C33 South, cm provides better comparison with the optical fluxes. The simplest interpretation of the data gives a radio spectral index of a = -0.89 with a break in the spectrum at log v ∼ 13.8. At optical frequencies, the spectral index is a = -1.97.sperse 发表于 2025-3-22 18:57:19
https://doi.org/10.1007/BFb0036008Neutrino; Quasar; active galactic nuclei; behavior; dynamics; galaxy; paper; photometry; relativistic jet; si含水层 发表于 2025-3-22 23:44:20
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