We derive the luminosity–temperature relation for the supercritically accreting black holes (BHs) and compare it to the data on ultraluminous X-ray sources (ULXs). At super-Eddington accretion rates, an outflow forms within the spherization radius. We construct the accretion disc model accounting fo...
Research Assistant
AI chat, annotations, notes & similar papers
No comments yet
Be the first to share your thoughts!