Abstract <p>Monitoring of 1–22 GHz spectra of blasars at the radio telescope RATAN-600 and their modeling using the known CATS data base are continued. The ‘‘Hedgehog’’ model proposed by N.S. Kardashev in 1969 and successfully applied later to explain variable spectra is used. For 13 objects modeled by relativistic proton jets, the main physical parameters were estimated. In 4 of them, new compact components in active nuclei may be detected. Accelerated protons may be high energy neutrino sources.</p>

错误:搜索内容不能为空,请输入英文关键词
错误:关键词超出字数限制,请精简
高级检索

Radio Structure of Active Galactic Nuclei on the RATAN-600 and CATS Data at Frequencies 0.01–500 GHz

  • Yu. A. Kovalev,
  • N. A. Nizhelsky,
  • Y. Y. Kovalev,
  • V. R. Amirkhanyan,
  • Yu. V. Sotnikova,
  • S. V. Troitsky,
  • A. V. Popkov,
  • A. V. Plavin,
  • A. K. Erkenov,
  • N. N. Bursov,
  • G. V. Zhekanis,
  • P. G. Tsibulev

摘要

Abstract

Monitoring of 1–22 GHz spectra of blasars at the radio telescope RATAN-600 and their modeling using the known CATS data base are continued. The ‘‘Hedgehog’’ model proposed by N.S. Kardashev in 1969 and successfully applied later to explain variable spectra is used. For 13 objects modeled by relativistic proton jets, the main physical parameters were estimated. In 4 of them, new compact components in active nuclei may be detected. Accelerated protons may be high energy neutrino sources.