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Surface Brightness Scale of Galactic Cepheids

Published online by Cambridge University Press:  25 May 2016

G. P. Di Benedetto
G. P. Di Benedetto*
Affiliation:
Istituto di Fisica Cosmica, Via Bassini 15, 20133 Milano, Italy

Abstract

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An accurate calibration of the surface brightness scale S V as a function of the near-IR color (V – K) has been recently measured for non-variable Galactic dwarf and giant stars. It can be shown that this correlation can be applied to the S V scale of Galactic Cepheid variable stars, which are of major cosmological interest.

Information

Type
Part 8. Cepheids and Distances
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999, pp. 561 - 562
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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