Alternate Names
Shklovskii, Iosif Samuilovich; Shklovskij, Iosif Samuilovich
Born Glukhov, (Ukraine), 1 July 1916
Died Moscow, (Russia), 3 March 1985
Theoretical astrophysicist Iosif S. Shklovsky was one of the most remarkable personalities and scholars among the Soviet astronomy community of his time. He chose as his own most important contributions the derivation of a reliable distance scale for planetary nebulae and the recognition that the emission from the Crab Nebula is synchrotron radiation (from which he predicted optical polarization, soon after found). Many would also mention his 1964 suggestion that the energy source for quasars is accretion of gas onto giant black holes at the centers of galaxies.
Following high school graduation, Shklovsky spent 2 years working in railroad construction, before beginning the study of physics and chemistry at the Far Eastern State University in Vladivostok, Russia, in 1933. He transferred to Moscow State University (MSU), completing a first...
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Selected References
Friedman, Herbert (1985). “Josif Samuilovich Shklovsky.” Physics Today 38, no. 5: 104–106.
Kardashev, N. S. (1992). Astrophysics on the Threshold of the 21st Century. Philadelphia: Gordon & Breach.
Shklovskii, I. S. and Carl Sagan (1966). Intelligent Life in the Universe. San Francisco: Holden-Day.
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— (1978). Stars, Their Birth, Life and Death. San Francisco: W. H. Freeman.
— (1991). Five Billion Vodka Bottles to the Moon: Tales of a Soviet Scientist. New York: W. W. Norton.
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Gurshtein, A.A. (2014). Shklovsky, Iosif Samuilovich. In: Hockey, T., et al. Biographical Encyclopedia of Astronomers. Springer, New York, NY. https://doi.org/10.1007/978-1-4419-9917-7_1276
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