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1. The White Dwarfs: Discovery and Observation
Published online by Cambridge University Press: 14 August 2015
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White dwarfs have been known for slightly more than fifty years; with their planetlike diameters, and stellar-like masses their densities are enormously much higher than those of ‘normal’ stars. They thus appear to represent a state of matter totally unknown and possibly unattainable on earth.
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- Research Article
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- Copyright © Reidel 1971
References
[5]
Chavira, E. and Iriarte, B.: 1957, Bol. Obs. Tac. y Ton., No. 16; also No. 18, 1959.Google Scholar
[12]
Kinman, T. D.: 1965, Astrophys. J.
142, 1241; also
Greenstein, J. L.: 1966, Astrophys. J. 144, 496.Google Scholar
[14]
Luyten, W. J.: 1969, Proper Motion Survey with the 48 inch Schmidt Telescope, No. XVIII.Google Scholar
[16]
Luyten, W. J.: 1956, A Search for Faint Blue Stars, No. VIII; also 1969, Proper Motion Survey with the 48 inch Schmidt Telescope, No. XVIII.Google Scholar
[22]
Van Rhijn, P. and Raimond, J. J.: 1934, Monthly Notices Roy. Astron. Soc.
94, 508.Google Scholar
[23]
Humason, M. L. and Zwicky, F.: 1947, Astrophys. J.
105, 85; also A Search for Faint Blue Stars, No. I, 1952.Google Scholar
[24]
Luyten, W. J.: 1969, Proper Motion Survey with the 48 inch Schmidt Telescope, No. XVII.Google Scholar
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