Tidal disruption jets of supermassive black holes as hidden sources of cosmic rays: Explaining the IceCube TeV-PeV neutrinos [PDF]
, 2016 Xiang‐Yu Wang, Ruo-Yu Liu
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The Astrophysical JournalYoung stars form in clusters within molecular clouds, but older stars are evenly distributed across the galactic disk, necessitating an explanation for cluster dissolution.
Xiao-Tong Chen, Guang-Xing Li
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Tidal Disruption of a Main-sequence Star by an Intermediate-mass Black Hole: A Bright Decade [PDF]
, 2018 Jin-Hong Chen, Rong-Feng Shen
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Repeating partial disruptions and two-body relaxation
The Open Journal of AstrophysicsTwo-body relaxation may drive stars onto near-radial orbits around a massive black hole, resulting in a tidal disruption event (TDE). In some circumstances, stars are unlikely to undergo a single terminal disruption, but rather to have a sequence of many
Luca Broggi +6 more
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Tidal disruption of a white dwarf by a black hole: the diversity of nucleosynthesis, explosion energy, and the fate of debris streams [PDF]
, 2018 Kojiro Kawana +2 more
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Micro–Tidal Disruption Events at Galactic Centers
The Astrophysical JournalThis work explores a scenario for micro–tidal disruption events (TDEs) triggered by close encounters between high-speed white dwarfs (WDs) and stellar-mass black holes (sBHs) in galactic centers.
Xinyu Li +3 more
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Tidal Disruption of Small Satellites Orbiting Black Holes [PDF]
, 2009 C. Germanà +5 more
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Modeling Tidal Disruptions with Dynamical Tides
The Astrophysical JournalTidal disruption events (TDEs) occur when stars pass close enough to supermassive black holes to be torn apart by tidal forces. Traditionally, these events are studied with computationally intensive hydrodynamical simulations. In this paper, we present a
Zihan Zhou +3 more
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Radio emission from the unbound debris of tidal disruption events. [PDF]
Mon Not R Astron Soc, 2019 Yalinewich A +3 more
europepmc +1 more source
The Influence of Central Body Tides on Catastrophic Disruptions of Close-in Planetary Satellites
The Astrophysical JournalWe model the outcomes of catastrophic disruptions on small, gravity-dominated natural satellites, accounting for the tidal potential of the central body, which is neglected in classical disruption scaling laws. We introduce the concept of ${Q}_{\,\rm{TD}\
Harrison Agrusa, Patrick Michel
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