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Implementation in FORTRAN of the NASA Breakup Model from the paper of Johnson et al. (2001) NASA's new breakup model of EVOLVE 4.0.
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This project contains the deveopment of the compose code only.
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Interface Fortran pour simplifier l'utilisation de HDF5
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The Stellar Parameters INferred Systematically (SPInS) characterises stars based on classic constraints. It has be derived from the AIMS code. For more details, see https://dreese.pages.obspm.fr/spins
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