Abstract
I review the theoretical and observational data supporting the existence of black holes at various mass scales and then give a brief account of the recent progress in the understanding of the stellar tidal disruption process, which is expected to play a prominent role in fuelling large black holes in galactic nuclei.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
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
