Nonthermal emissions from shocked shells driven by powerful agn jets

Hirotaka Ito, Motoki Kino, Nozomu Kawakatu, Shoichi Yamada

研究成果: Article


We explore the emissions by accelerated electrons in shocked shells driven by jets in active galactic nuclei (AGNs). Focusing on powerful sources which host luminous quasars, the synchrotron radiation and inverse-Compton (IC) scattering of various photons that are mainly produced in the core are considered as radiation processes. We show that the radiative output is dominated by the IC emission for compact sources (≲ 30 kpc), whereas the synchrotron radiation is more important for larger sources. It is predicted that, for powerful sources (Lj ∼ 1047 ergs s -1), GeV-TeV gamma-rays produced via the IC emissions can be detected by the Fermi satellite and modern Cherenkov telescopes such as MAGIC, HESS and VERITAS if the source is compact.

ジャーナルInternational Journal of Modern Physics D
出版物ステータスPublished - 2010 6 1

ASJC Scopus subject areas

  • Mathematical Physics
  • Astronomy and Astrophysics
  • Space and Planetary Science

フィンガープリント Nonthermal emissions from shocked shells driven by powerful agn jets' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

  • これを引用