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Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS):Library of Fallback Rates
- Source :
- Law-Smith, J A P, Coulter, D A, Guillochon, J, Mockler, B & Ramirez-Ruiz, E 2020, ' Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS) : Library of Fallback Rates ', Astrophysical Journal, vol. 905, no. 2, 141 . https://doi.org/10.3847/1538-4357/abc489
- Publication Year :
- 2020
-
Abstract
- We present the STARS library, a grid of tidal disruption event (TDE) simulations interpolated to provide the mass fallback rate ($dM/dt$) to the black hole for a main-sequence star of any stellar mass, stellar age, and impact parameter. We use a one-dimensional stellar evolution code to construct stars with accurate stellar structures and chemical abundances, then perform tidal disruption simulations in a three-dimensional adaptive-mesh hydrodynamics code with a Helmholtz equation of state, in unprecedented resolution: from 131 to 524 cells across the diameter of the star. The interpolated library of fallback rates is available on GitHub (https://github.com/jamielaw-smith/STARS_library) and version 1.0.0 is archived on Zenodo; one can query the library for any stellar mass, stellar age, and impact parameter. We provide new fitting formulae for important disruption quantities ($\beta_{\rm crit}, \Delta M, \dot M_{\rm peak}, t_{\rm peak}, n_\infty$) as a function of stellar mass, stellar age, and impact parameter. Each of these quantities vary significantly with stellar mass and stellar age, but we are able to reduce all of our simulations to a single relationship that depends only on stellar structure, characterized by a single parameter $\rho_c/\bar\rho$, and impact parameter $\beta$. We also find that, in general, more centrally concentrated stars have steeper $dM/dt$ rise slopes and shallower decay slopes. For the same $\Delta M$, the $dM/dt$ shape varies significantly with stellar mass, promising the potential determination of stellar properties from the TDE light curve alone. The $dM/dt$ shape depends strongly on stellar structure and to a certain extent stellar mass, meaning that fitting TDEs using this library offers a better opportunity to determine the nature of the disrupted star and the black hole.<br />Comment: 35 pages, 23 figures. Published in ApJ. v2: added Figure 23, references added, minor edits to text; v3: matches published version. Interpolated library of fallback rates is available at https://github.com/jamielaw-smith/STARS_library
- Subjects :
- 010504 meteorology & atmospheric sciences
Stellar mass
DISC FORMATION
FOS: Physical sciences
Galaxy nuclei
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Star (graph theory)
01 natural sciences
Tidal disruption event
HYDRODYNAMICS
SUPERMASSIVE BLACK-HOLES
0103 physical sciences
Astrophysics::Solar and Stellar Astrophysics
Stellar structure
Tidal disruption
MASSES
010303 astronomy & astrophysics
Stellar evolution
Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics::Galaxy Astrophysics
0105 earth and related environmental sciences
High Energy Astrophysical Phenomena (astro-ph.HE)
Physics
Main sequence stars
Astronomy and Astrophysics
CLUSTER
Black hole physics
Light curve
EVOLUTION
SIMULATIONS
GALAXIES
Stars
Astrophysics - Solar and Stellar Astrophysics
ENCOUNTERS
Space and Planetary Science
Active galaxies
COMPRESSION
Astrophysics::Earth and Planetary Astrophysics
Impact parameter
Astrophysics - High Energy Astrophysical Phenomena
Gravitation
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Law-Smith, J A P, Coulter, D A, Guillochon, J, Mockler, B & Ramirez-Ruiz, E 2020, ' Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS) : Library of Fallback Rates ', Astrophysical Journal, vol. 905, no. 2, 141 . https://doi.org/10.3847/1538-4357/abc489
- Accession number :
- edsair.doi.dedup.....e92b859dbde010d1b87f5b0927a19fca
- Full Text :
- https://doi.org/10.3847/1538-4357/abc489