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Strömgren, Bengt Georg Daniel (1908–1987)





Bengt Stromgren
Swedish astronomer who did important research in stellar structure in the 1930s but is best known for his work on ionized gas clouds – H II regions – around hot stars. He surveyed H II regions and found relations between the gas density, the luminosity of the star, and the size of the Strömgren sphere of ionized hydrogen around it. Son of the director of the Copenhagen University Observatory, Svante Strömgren (1870–1947), he had published many research papers, mostly in celestial mechanics, and coauthored a book by the time he received his Ph.D. from Copenhagen at age 21. After working there and at the Yerkes Observatory he succeeded his father at Copenhagen in 1940. He was director of Yerkes and McDonald Observatories from 1951 to 1957 and spent 10 years at the Institute for Advanced Study in Princeton before returning to Copenhagen.


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