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In 1930 Chandra, as he was always called, showed that a star of a mass greater than 1.4 times that of the Sun had to end its life by collapsing into an object of enormous density unlike any object known at that time. He said one is left speculating on other possibilities , namely objects such as black holes. For his work in this area he was awarded the Nobel prize for Physics in 1983. He described this work in The Mathematical Theory of Black Holes (1983).
His other books include Principles of Stellar Dynamics (1942), Hydrodynamic and Hydromagnetic Stability (1961), and Truth and Beauty: Aesthetics and Motivations in Science (1987). He was awarded the Royal Medal of the Royal Society in 1962. From 1952 until 1971 he was editor of the Astrophysical Journal .
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