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Optical spectral properties of radio loud quasars along the main sequence
Published online by Cambridge University Press: 29 January 2021
Abstract
We analyze the optical properties of Radio-Loud quasars along the Main Sequence (MS) of quasars. A sample of 355 quasars selected on the basis of radio detection was obtained by cross-matching the FIRST survey at 20cm and the SDSS DR12 spectroscopic survey. We consider the nature of powerful emission at the high-Fe ii end of the MS. At variance with the classical radio-loud sources which are located in the Population B domain of the MS optical plane, we found evidence indicating a thermal origin of the radio emission of the highly accreting quasars of Population A.
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- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 15 , Symposium S356: Nuclear Activity in Galaxies Across Cosmic Time , October 2019 , pp. 310 - 313
- Copyright
- © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union
Footnotes
Present address: Institute of Physics, University of Cologne, Germany