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Chandrasekhar limit |
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Chandrasekhar limit [ˌtʃændrəˈsiːkə]
n (Astronomy) Astronomy the upper limit to the mass of a white dwarf, equal to 1.44 solar masses. A star having a mass above this limit will continue to collapse to form a neutron star [named after Subrahmanyan Chandrasekhar (1910-95), Indian-born US astronomer, who calculated it]
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