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Does Every Quasar Harbor A Blazar?

Feng Ma·Beverley J. Wills
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Abstract

Assuming there is a blazar type continuum in every radio-loud quasar, we find that the free-free heating due to the beamed infrared continuum can greatly enhance collisionally excited lines, and thus explain the stronger CIV $λ$1549 line emission observed in radio loud quasars. We further predict that the CIV line should show variability {\it not} associated with observed continuum or Ly$α$ variability.

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Feng Ma, Beverley J. Wills. 1998-07-31. Does Every Quasar Harbor A Blazar?. https://doi.org/10.1086/311573

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