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Displaying 1 - 9 of total 9 results:
Early years; undergraduate at Harvard University, 1930-1934, and growth of interest in astronomy; graduate student and postdoctoral fellow at Harvard University, 1934-1941; social and scientific life, atomic physics work; Robert McMath and character of McMath-Hulbert observatory; mechanical engineering work in World War II; chairmanship of University of Michigan Astronomy Department, 1946-1960; optical and radio telescopes and funding; work on solar infrared and element abundances; Chairman and Director at Harvard, 1960-1971; relations with Smithsonian Institution, other politics, fund-rais
Early years; undergraduate at Harvard University, 1930-1934, and growth of interest in astronomy; graduate student and postdoctoral fellow at Harvard University, 1934-1941; social and scientific life, atomic physics work; Robert McMath and character of McMath-Hulbert observatory; mechanical engineering work in World War II; chairmanship of University of Michigan Astronomy Department, 1946-1960; optical and radio telescopes and funding; work on solar infrared and element abundances; Chairman and Director at Harvard, 1960-1971; relations with Smithsonian Institution, other politics, fund-rais
Early years; undergraduate at Harvard University, 1930-1934, and growth of interest in astronomy; graduate student and postdoctoral fellow at Harvard University, 1934-1941; social and scientific life, atomic physics work; Robert McMath and character of McMath-Hulbert observatory; mechanical engineering work in World War II; chairmanship of University of Michigan Astronomy Department, 1946-1960; optical and radio telescopes and funding; work on solar infrared and element abundances; Chairman and Director at Harvard, 1960-1971; relations with Smithsonian Institution, other politics, fund-rais
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Childhood on Missouri farm, early education and interest in science. Enters University of Missouri, 1907; B.A., 1910, M.A., 1911; influence of Oliver Kellogg, Eli Haines, Frederick Seares. To Princeton University, 1911-1914; first doctoral student of Henry Norris Russell; close relationship with Russell, impressions of him as teacher, co-worker, and friend; works on orbits of eclipsing binaries and Cepheid variable star theory; Russell’s experiments with darkening at the limb; Shapley’s research methods, requirements for doctorate in astronomy, 1910; Robert W. Wood, R. S. Dugan, O. W.
Childhood on Missouri farm, early education and interest in science. Enters University of Missouri, 1907; B.A., 1910, M.A. 1911; influence of Oliver Kellogg, Eli Haines, Frederick Seares. To Princeton University, 1911-1914; first doctoral student of Henry Norris Russell; close relationship with Russell, impressions of him as teacher, co-worker, and friend; works on orbits of eclipsing binaries and Cepheid variable star theory; Russell’s experiments with darkening at the limb; Shapley’s research methods, requirements for doctorate in astronomy, 1910; Robert W. Wood, R. S. Dugan, O. W.