Input files needed to reproduce the simulations as well as output MESA history files (i.e. stellar tracks) to paper "Massive donors in interacting binaries: impact of metallicity". MESA version r11554. Output history files are provided for the models with the chosen reference set of input physical assumptions. History files from other models discussed in the paper can be provided upon request
We have included the inlists, important run files, and selected simulation data accompanying Rui and...
Associated MESA (r11701) inlists, source files (run_star_extras.f90 and run_binary_extras.f), and ou...
Binary systems are important probes of the origin of stars with peculiar chemical features through t...
Input files needed to reproduce the simulations as well as output MESA history files (i.e. stellar t...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
MESA inlists, run_star_extras, and data associated with Marchant et al. (2017). MESA version 8118. ...
Model data and input files (inlists) used to compute MESA binary models to paper "Partial-envelope s...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
Metallicity is known to significantly affect the radial expansion of a massive star: the lower the m...
Context. The majority of massive stars are part of binary systems. In about a quarter of these, the ...
================================================================================ Title: Aluminium-26...
Data products and files to reproduce the results from du Buisson et al. (2020). MESA Calculations ...
Binary model inlists for MESA, as used for the paper Coping with loss: Stability of mass transfer fr...
Input files and simulation results for stellar evolution tracks computed for the paper "The excess o...
This repository contains the datasets from the original smoothed particle hydrodynamics (SPH) calcul...
We have included the inlists, important run files, and selected simulation data accompanying Rui and...
Associated MESA (r11701) inlists, source files (run_star_extras.f90 and run_binary_extras.f), and ou...
Binary systems are important probes of the origin of stars with peculiar chemical features through t...
Input files needed to reproduce the simulations as well as output MESA history files (i.e. stellar t...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
MESA inlists, run_star_extras, and data associated with Marchant et al. (2017). MESA version 8118. ...
Model data and input files (inlists) used to compute MESA binary models to paper "Partial-envelope s...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
Metallicity is known to significantly affect the radial expansion of a massive star: the lower the m...
Context. The majority of massive stars are part of binary systems. In about a quarter of these, the ...
================================================================================ Title: Aluminium-26...
Data products and files to reproduce the results from du Buisson et al. (2020). MESA Calculations ...
Binary model inlists for MESA, as used for the paper Coping with loss: Stability of mass transfer fr...
Input files and simulation results for stellar evolution tracks computed for the paper "The excess o...
This repository contains the datasets from the original smoothed particle hydrodynamics (SPH) calcul...
We have included the inlists, important run files, and selected simulation data accompanying Rui and...
Associated MESA (r11701) inlists, source files (run_star_extras.f90 and run_binary_extras.f), and ou...
Binary systems are important probes of the origin of stars with peculiar chemical features through t...