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Secondary electron production and the millimeter to gamma-ray continuum of emission-line quasi-stellar objects

Journal Article · · Astrophysical Journal; (USA)
DOI:https://doi.org/10.1086/168328· OSTI ID:7135145
;  [1]
  1. Minnesota Univ., Minneapolis (USA)
A model is outlined to explain the multifrequency continua of active galactic nucleus (AGN) and QSOs based on synchrotron and Compton emission of secondary electrons. 3C 273 is used as a particular guide for observational constraints since it so well observed from radio to gamma-ray photon energies. In this model the large blue bump and blue bump Compton components arise in the innermost region near a supermassive compact object with strong magnetic field. Infrared synchrotron emission and infrared Compton components arise in the low-field region. The model results in bumps, wiggles, and inflections in the multifrequency continuum that correspond to those observed. 47 refs.
OSTI ID:
7135145
Journal Information:
Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 349; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English