0.35-3.5 micron photometry of X-ray emitting QSOs

Details 0.35-3.5 micron photometry of X-ray emitting QSOs 0.35-3.5 micron photometry of X-ray emitting QSOs

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...259..486s&link_type=abstract

Astrophysical Journal, Part 1, vol. 259, Aug. 15, 1982, p. 486-494. NSF-supported research.

Astronomy and Astrophysics

Astronomy

35

Astronomical Photometry, Infrared Astronomy, Quasars, Synchrotron Radiation, Visible Spectrum, X Ray Sources, Bl Lacertae Objects, Compton Effect, Infrared Photometry, Infrared Spectra, Nonthermal Radiation, Particle Flux Density, Photons, Spectral Energy Distribution, Thermal Emission

Scientific paper

Visual and infrared photometry of X-ray emitting QSOs is reported. The strongest emitters of X-ray relative to visual emission are those with the strongest nonthermal visual-infrared emission. This result is most easily explained if the X-rays are Compton-scattered photons of lower initial frequency rather than a simple extrapolation of the visual-infrared spectrum into the X-ray region.

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