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Subrahmanyan Chandrasekhar. Subrahmanyan Chandrasekhar Aussprache ⓘ /? (* 19. Oktober 1910 in Lahore, Britisch-Indien; † 21. August 1995 in Chicago) war US-amerikanischer (Astro-)Physiker indischer Herkunft und 1983 Nobelpreisträger für Physik
Subrahmanyan Chandrasekhar FRS (/ ˌ tʃ æ n d r ə ˈ ʃ eɪ k ər /; 19 October 1910 – 21 August 1995) was an Indian-American theoretical physicist who made significant contributions to understanding of stellar evolution, black holes, and the structure of stars.
30. Apr. 2024 · Subrahmanyan Chandrasekhar (born October 19, 1910, Lahore, India [now in Pakistan]—died August 21, 1995, Chicago, Illinois, U.S.) was an Indian-born American astrophysicist who, with William A. Fowler, won the 1983 Nobel Prize for Physics for key discoveries that led to the currently accepted theory on the later evolutionary stages ...
- The Editors of Encyclopaedia Britannica
The Nobel Prize in Physics 1983 was divided equally between Subrahmanyan Chandrasekhar "for his theoretical studies of the physical processes of importance to the structure and evolution of the stars" and William Alfred Fowler "for his theoretical and experimental studies of the nuclear reactions of importance in the formation of the chemical ...
21. Aug. 1995 · Subrahmanyan Chandrasekhar The Nobel Prize in Physics 1983. Born: 19 October 1910, Lahore, India (now Pakistan) Died: 21 August 1995, Chicago, IL, USA. Affiliation at the time of the award: University of Chicago, Chicago, IL, USA.
29. Sept. 2023 · Subrahmanyan Chandrasekhar and William Alfred Fowler shared the Nobel Prize in Physics in 1983, for their work on stellar evolution. Although they were born just months apart, and died in the...
Trained as a physicist at Presidency College, in Madras, India and at the University of Cambridge, in England, he was one of the first scientists to combine the disciplines of physics and astronomy. Early in his career he demonstrated that there is an upper limit — now called the Chandrasekhar limit — to the mass of a white dwarf star. A ...
