Radio spectra and morphology of Radio-Loud Broad Absorption Line Quasars

Mathematics – Logic

Scientific paper

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Scientific paper

About 15% of the quasar population show broad absorption lines in their spectra generated from outflows with velocities up to 0.2 c. We selected a complete sample of Radio Loud Broad Absorption Line Quasars from the Sloan Digital Sky Survey, in order to study their spectral properties and orientation features at radio wavelengths. At the moment two models have been presented to explain these objects: an orientation model (Elvis 2000) and an evolutionary scenario (Becker et al. 2000). Results from our radio campaign will be presented, focusing on the spectral and morphological properties that can discriminate between the two models.

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