Authors:
Perez, E.;Penston, M. V.;Tadhunter, C.;Mediavilla, E.;Moles, M.
Journal:
Monthly Notices of the Royal Astronomical Society
Abstract:
The permitted broad component of the Hβ emission line in the broadline radio galaxy (BLRG) 3C390.3 presents a double-peaked structure, similar to that seen in cataclysmic variables. The profile of the line is well fitted by a relativistic accretion disc with an intermediate inclination to the line-of-sight.
URL:
https://ui.adsabs.harvard.edu/#abs/1988MNRAS.230..353P/abstract
Keywords:
Accretion Disks;Cataclysmic Variables;H Beta Line;Radio Galaxies;Astronomical Spectroscopy;Data Reduction;Energy Distribution;Ultraviolet Radiation;Astrophysics