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        "description": "The two-page paper gives approximately 0.91 solar masses under its stated composition assumption, including a molecular weight of 2.5. Substituting the later familiar numerical value would misrepresent this source. The result concerns the idealized model and compares earlier Stoner estimates; it does not establish the fate of every massive star. The cited original text supports this scoped reading; a local source copy is not distributed. No calculation was replayed.",
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      "statement": "# Chandrasekhar: the maximum mass of ideal white dwarfs\n\nCombined relativistic electron degeneracy with a polytropic stellar model to obtain an upper mass for an ideal white dwarf.\n\n## Scientific scope\n\nThe two-page paper gives approximately 0.91 solar masses under its stated composition assumption, including a molecular weight of 2.5. Substituting the later familiar numerical value would misrepresent this source. The result concerns the idealized model and compares earlier Stoner estimates; it does not establish the fate of every massive star. The cited original text supports this scoped reading; a local source copy is not distributed. No calculation was replayed.\n\n## Reading status\n\nThis is a source-linked WRS catalogue note. A full explanatory guide and independent scientific reconstruction have not been completed for this entry. Read the identified original work for its complete narrative and arguments.\n\n## People and systems\n\nS. Chandrasekhar\n\nListed source contributors; individual labor shares are not measured\n\n\n\n## Original sources\n\n- [Chandrasekhar, The Maximum Mass of Ideal White Dwarfs, Astrophysical Journal 74, 81–82 (1931); DOI 10.1086/143324](https://articles.adsabs.harvard.edu/pdf/1931ApJ....74...81C)\n",
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