Far-infrared intense-field phenomena in active galactic nuclei

Details Far-infrared intense-field phenomena in active galactic nuclei Far-infrared intense-field phenomena in active galactic nuclei

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985infph..25..521r&link_type=abstract

(European Physical Society, International Conference on Infrared Physics, 3rd, Zurich, Switzerland, July 23-27, 1984) Infrared P

Physics

Active Galactic Nuclei, Bl Lacertae Objects, Electromagnetic Interactions, Far Infrared Radiation, Line Spectra, Quasars, Charged Particles, Doppler Effect, Electrodynamics, Red Shift

Scientific paper

A major feature of many active galactic nuclei is that the bulk of their luminosity occurs in the FIR. This fact, combined with the small size of the objects, means that nonperturbative intense-field behavior is likely to exist at long wavelengths, even though visible and UV behavior is perturbative. The FIR can then cause unusual spectral phenomena. One example is significant broadening of spectral lines in quasars, and another is the absence of line spectra in BL Lac objects.

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