LOWER LIMIT. “An otherwise quiet MBH would show bright, beamed emission after the disruption of a WD. Therefore, detecting (or not detecting) signals from the tidal disruptions of WDs could place constraints on the MBH population.” (WD = white dwarf; MBH = Massive Black Hole).
https://lnkd.in/djnsGi4
linkedin post 2022-06-29 05:12:48
Nigel Fleming
September 21, 2022