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The Cepheid Luminosity Scale

Published online by Cambridge University Press:  12 April 2016

Edward G. Schmidt*
Affiliation:
Behlen Observatory, The University of Nebraska, Lincoln, NE 68588-0111

Extract

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The distances of clusters containing classical Cepheids are central to the calibration of the period-luminosity relation. As a step in improving the reliability of the calibration, uvbys photometry was obtained for B stars in eight of these clusters. These data were then used to determine the distances of the clusters and, thus, the absolute magnitudes of the Cepheids and the zero point of the PLC relation (See Schmidt 1984 for details).

Type
Part III. Extragalactic Cepheids and the PL Relation
Copyright
Copyright © Cambridge University Press 1985

References

Balona, L. A. and Shobbrook, R. R. 1984, preprint.Google Scholar
Barnes, T. G. 1979 In Highlights of Astronomy Vol 5 (Dordrecht: Reidel) p. 479 Google Scholar
Caldwell, J. A.R. 1983, Observatory 103, 244.Google Scholar
Cox, A. N. 1979, Ap. J. 229, 212.10.1086/156947CrossRefGoogle Scholar
de Vaucouleurs, 1978, Ap. J. 223, 351.10.1086/156269CrossRefGoogle Scholar
Fernie, J. D. and McGonegal, R. 1983, Ap. J. 275, 732.10.1086/161570CrossRefGoogle Scholar
Martin, W. L., Warren, P. R. and Feast, M. W. 1979, M.N.R.A.S. 188, 139.10.1093/mnras/188.1.139CrossRefGoogle Scholar
Pel, J. W. 1978, Astron. and Ap. 62, 75.Google Scholar
Sandage, A. and Tammann, G. A. 1969, Ap. J. 157, 683.10.1086/150106CrossRefGoogle Scholar
Schmidt, , 1984, Ap. J. (in press).Google Scholar
Stothers, R. B. 1983, Ap. J. 274, 20.10.1086/161422CrossRefGoogle Scholar
van den Bergh, S. 1976, in IAU Colloquium No. 37, p. 13.Google Scholar