Abstract
Indian-American theoretical astrophysicist S. Chandrasekhar shared the 1983 Nobel Prize in Physics (with William Fowler) for work done in the 1930s, which established an absolute upper mass limit, now called the Chandrasekhar limit, for an astronomical object in which the pressure support comes from electrons being crowded as closely together as quantum mechanics permits. This limit applies to white dwarf stars, such as the Sun will eventually become, and to the cores of more massive stars that then collapse into neutron stars or black holes.
Roy H. Garstang: deceased.
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Selected References
Garstang, R.H. 1997. Subrahmanyan Chandrasekhar (1910–1995). Publications of the Astronomical Society of the Pacific 109: 73–77.
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Garstang, R.H. (2022). Chandrasekhar, Subrahmanyan. In: Nicholson, P.D., Bartlett, J.L. (eds) Biographical Encyclopedia of Astronomers. Springer, New York, NY. https://doi.org/10.1007/978-1-0716-0738-1_263-5
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DOI: https://doi.org/10.1007/978-1-0716-0738-1_263-5
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Chandrasekhar, Subrahmanyan- Published:
- 29 June 2022
DOI: https://doi.org/10.1007/978-1-0716-0738-1_263-5
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Chandrasekhar, Subrahmanyan- Published:
- 22 January 2021
DOI: https://doi.org/10.1007/978-1-0716-0738-1_263-4