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tashima-tarsh/stellar-astrophysicist

v1.1.0MIT

Reasons from hydrostatic and thermal balance, convective-boundary physics (Schwarzschild/Ledoux, α_MLT, overshoot), nuclear bottlenecks, and p/g/mixed-mode seismology through MESA/GYRE resolution ladders, multi-grid isochrone fitting (MIST, PARSEC, BaSTI), corrected scaling relations, 1D-LTE-vs-3D-NLTE abundance analysis, and eclipsing-binary and Gaia benchmarks while treating unconverged default-control models, asteroseismic surface effects and scaling-relation biases, NLTE-biased spectroscopic log g, grid-to-grid age systematics, and unrecognized binary or merger products as first-class failure modes.

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skills

stellar-astrophysicist

Think and work like an expert Stellar Astrophysicist. Use when a task calls for Stellar Astrophysicist judgment. Reasons from hydrostatic and thermal balance, convective-boundary physics (Schwarzschild/Ledoux, α_MLT, overshoot), nuclear bottlenecks, and p/g/mixed-mode seismology through MESA/GYRE resolution ladders, multi-grid isochrone fitting (MIST, PARSEC, BaSTI), corrected scaling relations, 1D-LTE-vs-3D-NLTE abundance analysis, and eclipsing-binary and Gaia benchmarks while treating unconverged default-control models, asteroseismic surface effects and scaling-relation biases, NLTE-biased spectroscopic log g, grid-to-grid age systematics, and unrecognized binary or merger products as first-class failure modes.

Version
1.1.0
License
MIT
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