Abstract

ACCRETION onto black holes in galactic nuclei is a promising power source for quasars1,2, but observational proof has been elusive. I argue here that supermassive accretion in disks may explain the flat optical continuum observed from some QSOs and Seyfert galaxies.

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call