No CrossRef data available.
Article contents
The Cepheid Luminosity Scale
Published online by Cambridge University Press: 12 April 2016
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
The distance moduli of galactic clusters containing classical Cepheids are being redetermined using the four-color and Hβ photometric system. The results for four clusters are presented here and it is found that the distance moduli are smaller than previous values. Possible reasons for this discrepancy are discussed.
- Type
- V. Cepheids of Populations I and II
- Information
- International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 449 - 455
- Copyright
- Copyright © Reidel 1980
References
Fricke, K., Stobie, R.S., and Strittmatter, P.A.: 1972, Astrophys. J.
171, p. 593.CrossRefGoogle Scholar
Hansen, R.B.: 1980, in “Star Clusters” IAU Symp. No. 85, ed. Hesser, J.E. (Dordrecht: D. Reidel) p. 71.Google Scholar
King, D.S., Hansen, E.J., Ross, R.R., Cox, J.P.: 1975, Astrophys. J.
195, p. 467.CrossRefGoogle Scholar