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Published in 2021 at "Physical Review D"
DOI: 10.1103/physrevd.104.103019
Abstract: Stars that approach a supermassive black hole (SMBH) too closely can be disrupted by the tidal gravitational field of the SMBH. The resulting debris forms a tidal stream orbiting the SMBH which can collide with…
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Keywords:
tidal stream;
supermassive black;
two regimes;
circularization ... See more keywords