MESA inlists associated with Jones et al. (2015). MESA version 3709. Publication DOI: 10.1093/mnras/stu2657 Files are also available in a gihub repository her
Core-collapsed Supernova (CCSN) is one of violent phenomena in the universe. CCSN generates heavy el...
Massive stars can shed material via steady, line-driven winds, eruptive outflows, or mass transfer o...
MESA inlists associated with Fields et al. (2018). MESA version 7624. Publication DOI: 10.3847/1538...
Massive stars are key sources of radiative, kinetic, and chemical feedback in the universe. Grids of...
Massive stars are key sources of radiative, kinetic, and chemical feedback in the universe. Grids of...
Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of ...
Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of ...
Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of ...
This is a basic reproduction package for the paper "Different to the core: the pre-supernova structu...
This is a basic reproduction package for the paper "Different to the core: the pre-supernova structu...
This is a basic reproduction package for the paper "Different to the core: the pre-supernova structu...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
MESA inlists for the simulation described in https://arxiv.org/abs/1901.04512. This uses MESA versio...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
We substantially update the capabilities of the open source software package Modules for Experiments...
Core-collapsed Supernova (CCSN) is one of violent phenomena in the universe. CCSN generates heavy el...
Massive stars can shed material via steady, line-driven winds, eruptive outflows, or mass transfer o...
MESA inlists associated with Fields et al. (2018). MESA version 7624. Publication DOI: 10.3847/1538...
Massive stars are key sources of radiative, kinetic, and chemical feedback in the universe. Grids of...
Massive stars are key sources of radiative, kinetic, and chemical feedback in the universe. Grids of...
Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of ...
Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of ...
Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of ...
This is a basic reproduction package for the paper "Different to the core: the pre-supernova structu...
This is a basic reproduction package for the paper "Different to the core: the pre-supernova structu...
This is a basic reproduction package for the paper "Different to the core: the pre-supernova structu...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
MESA inlists for the simulation described in https://arxiv.org/abs/1901.04512. This uses MESA versio...
Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium st...
We substantially update the capabilities of the open source software package Modules for Experiments...
Core-collapsed Supernova (CCSN) is one of violent phenomena in the universe. CCSN generates heavy el...
Massive stars can shed material via steady, line-driven winds, eruptive outflows, or mass transfer o...
MESA inlists associated with Fields et al. (2018). MESA version 7624. Publication DOI: 10.3847/1538...