Results 1 to 10 of about 1,263,228 (294)

The γ-ray afterglows of tidal disruption events. [PDF]

open access: yesMon Not R Astron Soc, 2016
A star wandering too close to a supermassive black hole (SMBH) will be tidally disrupted. Previous studies of such "tidal disruption event" (TDE) mostly focus on the stellar debris that are bound to the system, because they give rise to luminous flares.
Chen X, Gómez-Vargas GA, Guillochon J.
europepmc   +6 more sources

Tidal dissipation and evolution of white dwarfs around massive black holes: an eccentric path to tidal disruption

open access: yes, 2019
<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2017MNRAS.468.2296V">Tidal dissipation and evolution of white dwarfs around massive black holes: an eccentric path to tidal disruption</a></p ...
Vick, Michelle (6455615)   +5 more
core   +1 more source

Demographics of tidal disruption events with

open access: yes
Stars can be ripped apart by tidal forces in the vicinity of a massive black hole (MBH), causing luminous flares known as tidal disruption events (TDEs). These events could be contributing to the mass growth of intermediate-mass MBHs.
L. Broggi   +7 more
core   +1 more source

Radio emission from the unbound debris of tidal disruption events. [PDF]

open access: yesMon Not R Astron Soc, 2019
Yalinewich A   +3 more
europepmc   +1 more source

SIFTING FOR SAPPHIRES: SYSTEMATIC SELECTION OF TIDAL DISRUPTION EVENTS IN iPTF. [PDF]

open access: yesAstrophys J Suppl Ser, 2018
Hung T   +17 more
europepmc   +1 more source

Optical discovery of a relativistic jet from the tidal disruption of a star by a supermassive black hole

open access: yes, 2022
Andreoni I   +76 more
europepmc   +1 more source

Tidal dissipation and evolution of white dwarfs around massive black holes: an eccentric path to tidal disruption [PDF]

open access: yes, 2017
A white dwarf (WD) captured into a high-eccentricity orbit around a massive black hole (MBH) may undergo many pericentre passages before tidal disruption. During these passages, the tidal potential of the MBH excites internal oscillations or waves in the
Lai, Dong, Vick, Michelle, Fuller, Jim
core  

Tidal Disruption of a Star on a Nearly Circular Orbit

open access: yes
We consider Roche lobe overflow (RLO) from a low-mass star on a nearly circular orbit, onto a supermassive black hole (SMBH). If mass transfer is unstable, its rate accelerates in a runaway process, resulting in highly super-Eddington mass accretion ...
Itai Linial, Eliot Quataert
core   +1 more source

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