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The Cepheid Distance Scale: A History |
1.1:
Henrietta Leavitt’s Cepheid Variable Observations1.2:
Hertzsprung’s First Cepheid Distance Scale Calibration : The Great debate and the Great mistake: Shapley, Hubble, Baade
2.1:
A new Cepheid calibration by Shapley2.2:
Extragalactic distances obtained with Cepheid Variables2.3:
The Great Mistake: Two Cepheid populations Cepheid Period-Luminosity-Colour Relations: 1952-1980s3.1:
Semi-theoretical Approaches3.2:
PLC versus PL relations for Cepheids3.3:
Reddening and colour terms3.4:
A few notes on metallicity in Cepheids3.5
: Two Further Cepheid Calibrations The Modern Era4.1:
A New Emphasis in Cepheid Calibration4.2:
Demise of the PLC relation for Cepheids?4.3:
Multiwavelength Observations: CCD and near IR Coverage of Cepheids and other Variable Stars4.4:
Metallicity of Variable Stars4.5:
Hipparcos and the Cepheid zero-point calibrationConcluding Remarks on the Cepheid Distance Scale
A computer model of the PL relation for CepheidsAbout this site
The Cepheid Distance Scale: A history is based upon a dissertation presented towards the award of MSc (astrophysics) at Queen Mary College, University of London. The original text contained extensive footnotes which have been removed for the sake of simplicity. They nevertheless clarified, and in many cases justified, certain points made in the text. If you have any questions or disagreements please e-mail me. I might be able to resolve these by coding some of the original footnotes back in.
Acknowledgements
Thanks to the American Association of Variable Star Observers for providing copies of the original Leavitt papers, and the library of the Royal Astronomical Society London for obtaining Hertzsprung’s early work. Extensive use has also been made of NASA's Astrophysics Data System Bibliographic Services.
Copyright Notice
The Cepheid Distance Scale: A History ã Nick Allen AGSM BA BEd MSc FRAS MInstPI 2001
Link to this site
Last Updated: May 2009