Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..545s&link_type=abstract
HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo
Astronomy and Astrophysics
Astronomy
Radio Galaxies, Elliptical Galaxies, Gamma-Ray Sources, Gamma-Ray Bursts, Jets And Bursts, Galactic Winds And Fountains
Scientific paper
Several low-power kiloparsec-scale jets in nearby radio galaxies are known for their synchrotron radiation extending up to optical and X-ray photon energies. Here we comment on the high-energy γ-ray emission of such objects, resulting from comptonization of the starlight photon field of the host galaxies by the synchrotron-emitting jet electrons. Particular case of radio galaxy M 87 is analysed in more details, including relativistic bulk velocity of the jet as well as the Klein-Nishina effects. We show, that present upper limits for such an emission imposed by Whipple observations imply that the magnetic field in the brightest knot A of M 87 jet cannot be smaller than the equipartition value. We also comment on the regular (non-active) galaxy NGC 821, for which kpc-scale jet-like feature has been recently discovered in X-rays by Chandra. We conclude, that if the interpretation of this feature as the synchrotron-emitting jet-like outflow is correct, nearby elliptical galaxies can constitute an important class of the extragalactic sources of high energy (from GeV up to TeV) γ-ray radiation detectable by the future Cherenkov Telescopes and GLAST.
Ostrowski Marcin
Siemiginowska Aneta
Sikora Marcin
Stawarz Łukasz
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