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7. The Cepheid Distance Scale and Galactic Kinematic Parameters

Published online by Cambridge University Press:  25 April 2016

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Cepheid variables have long been a primary source of knowledge of galactic distances. It is therefore important to examine critically the accuracy of the cepheid distance scale to determine whether it is adequate for present needs. Proper motions resulting from the solar motion provide a fundamental determination of the distance scale, according to the well-known formula

Type
Research Article
Copyright
Copyright © Cambridge University Press 1960

References

[1] Shapley, H. Proc. Nat. Acad. Sci. 9, 541, 1940.Google Scholar
[2] Blaauw, A. and Morgan, H. R. B.A.N. 12, 95, 1954.Google Scholar
[3] Eggen, O. J., Gascoigne, S. C. B. and Burr, E. J. M.N.R.A.S. 117, 406, 1957.CrossRefGoogle Scholar
[4] Kron, G. E. and Svolopoulos, S. (These proceedings.)Google Scholar
[5] Eggen, O. J. Ap. J. 113, 367, 1951.Google Scholar
[6] Code, A. D. Charlottesville Conference on the Cosmic Distance Scale, 1956.Google Scholar
[7] Stibbs, D. W. N. M.N.R.A.S. 115, 323, 1955.Google Scholar
[8] Gascoigne, S. C. B. and Eggen, O. J. M.N.R.A.S. 117, 430, 1957.Google Scholar
[9] Walraven, Th., Muller, A. B. and Oosterhoff, P. Th. B.A.N. 14, 81, 1958.Google Scholar
[10] Schmidt, T. Z. Ap. 45, 214, 1958.Google Scholar
[11] Kraft, R. P. (See Irwin's paper in these proceedings.)Google Scholar