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Local Distance Indicators

Published online by Cambridge University Press:  26 May 2016

Michael. Feast
Michael. Feast*
Affiliation:
Astronomy Department, University of Cape Town, Rondebosch, 7701, South Africa, email: [email protected]

Abstract

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A summary is given of the calibration of the Cepheid scale required in the derivation of distances from observations at V and I, as in the HST work on extragalactic Cepheids. There is some evidence that a small metallicity correction may be necessary in deriving distances in this way. The evidence for this comes both from observations of Cepheids of different metallicities and from a comparison of the LMC distance modulus derived from Cepheids and that derived by other methods.

Type
Part VI: Determination of H0
Information
Symposium - International Astronomical Union , Volume 201: New Cosmological Data and the Values of the Fundamental Parameters , 2005 , pp. 181 - 189
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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