The interplay among accretion power, ionizing continuum, and outflows in quasars at Cosmic noon.
Abstract
Optical and UV spectroscopy of very powerful quasars offers invaluable insights into both accretion properties and sub-pc to kpc-scale ionized gas kinematics of objects hosting the most extreme SMBHs.
Fields of Study & Subjects
Galaxies: Formation
Evolution
Phenomena
Astrophysical Phenomena and Observations
Astrophysics and Star Formation Studies
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 27 February 2026
- Language
- EN