H. R. Chandrasekhar is likely a reference to Homi R. Chandrasekhar, an accomplished Indian astrophysicist, who is known for his work in the field of astrophysics and related areas. He is most notable for his contributions to the study of stellar structures and evolution, including the Chandrasekhar limit, which defines the maximum mass of a stable white dwarf star. The Chandrasekhar limit is approximately 1.
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