Does Every Quasar Harbor a Blazar?
Author(s) -
Feng Ma,
Beverley J. Wills
Publication year - 1998
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/311573
Subject(s) - quasar , blazar , astrophysics , physics , emission spectrum , line (geometry) , astronomy , spectral line , galaxy , gamma ray , geometry , mathematics
Assuming there is a blazar type continuum in every radio-loud quasar, we findthat the free-free heating due to the beamed infrared continuum can greatlyenhance collisionally excited lines, and thus explain the stronger CIV$\lambda$1549 line emission observed in radio loud quasars. We further predictthat the CIV line should show variability {\it not} associated with observedcontinuum or Ly$\alpha$ variability.Comment: 15 pages, 3 figures; to appear in Astrophys. J. Let
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