The infrared emission of quasars

Details The infrared emission of quasars The infrared emission of quasars

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111...97c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 1, April 1985, p. 97-102. Research supported by the Conselho Naci

Astronomy and Astrophysics

Astronomy

Astronomical Models, Infrared Astronomy, Quasars, Radio Emission, Submillimeter Waves, Flux Density, Injection, Relativistic Particles, Synchrotron Radiation

Scientific paper

A model of two compact components (one contributes at radio and submillimeter wavelength and the other is very small and emits at the infrared region) is proposed to interpret the spectrum of quasi-stellar objects at radio and infrared wavelengths. The physical parameters are estimated from the observed data of 3C 273 for the author's model and for the model which is derived by assuming the infrared emission as an extrapolation of the synchrotron radio source. It is proved that the author's model can explain the observational spectra, while the other model has some difficulties to interpret them completely.

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