MESA inlist files for the paper "The mass fallback rate in relativistic stellar tidal disruption events". Versions 15140 of MESA and MESA SDK 20.3.1 were used for the simulations. More details are in the README.txt file and in the paper
The tidal disruption of a star by a supermassive black hole, and the subsequent accretion of the dis...
Input files (inlists) used to compute MESA binary models to paper "Partial-envelope stripping and nu...
International audienceThe rate of tidal disruption events (TDEs) depends sensitively on the stellar ...
Highly energetic stellar tidal disruption events (TDEs) provide a way to study black hole characteri...
The tidal disruption of stars by supermassive black holes (SMBHs) can be used to probe the SMBH mass...
A tidal disruption event (TDE) occurs when a star plunges through a supermassive black hole's tidal ...
Tidal disruption of stars in dense nuclear star clusters containing supermassive central black holes...
Input and output files of MESA and STELLA associated with the published journal article Balaji et al...
In this thesis I present numerical simulations of the tidal disruption of stars by supermassive blac...
Tidal disruption of stars in dense nuclear star clusters containing supermassive central black holes...
We present the STARS library, a grid of tidal disruption event (TDE) simulations interpolated to pro...
After the tidal disruption of a star by a massive black hole, disrupted stellar debris can fall back...
Binary model inlists for MESA, as used for the paper Coping with loss: Stability of mass transfer fr...
A star whose orbit takes it on a suffciently close approach to a massive black hole (BH) will be shr...
The rate of tidal disruption events (TDEs), R-TDE, is predicted to depend on stellar conditions near...
The tidal disruption of a star by a supermassive black hole, and the subsequent accretion of the dis...
Input files (inlists) used to compute MESA binary models to paper "Partial-envelope stripping and nu...
International audienceThe rate of tidal disruption events (TDEs) depends sensitively on the stellar ...
Highly energetic stellar tidal disruption events (TDEs) provide a way to study black hole characteri...
The tidal disruption of stars by supermassive black holes (SMBHs) can be used to probe the SMBH mass...
A tidal disruption event (TDE) occurs when a star plunges through a supermassive black hole's tidal ...
Tidal disruption of stars in dense nuclear star clusters containing supermassive central black holes...
Input and output files of MESA and STELLA associated with the published journal article Balaji et al...
In this thesis I present numerical simulations of the tidal disruption of stars by supermassive blac...
Tidal disruption of stars in dense nuclear star clusters containing supermassive central black holes...
We present the STARS library, a grid of tidal disruption event (TDE) simulations interpolated to pro...
After the tidal disruption of a star by a massive black hole, disrupted stellar debris can fall back...
Binary model inlists for MESA, as used for the paper Coping with loss: Stability of mass transfer fr...
A star whose orbit takes it on a suffciently close approach to a massive black hole (BH) will be shr...
The rate of tidal disruption events (TDEs), R-TDE, is predicted to depend on stellar conditions near...
The tidal disruption of a star by a supermassive black hole, and the subsequent accretion of the dis...
Input files (inlists) used to compute MESA binary models to paper "Partial-envelope stripping and nu...
International audienceThe rate of tidal disruption events (TDEs) depends sensitively on the stellar ...
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