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Distances and Radii of Classical Cepheids

Published online by Cambridge University Press:  12 April 2016

T. G. Barnes III
Affiliation:
The University of Texas at Austin, Austin, Texas 78712 USA
T. J. Moffett
Affiliation:
Purdue University, West Lafayette, Indiana 47907 USA

Extract

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We have used new BVRI photometry and radial velocities of a selection of bright classical Cepheids to determine their distances and radii through the surface brightness method. The improved photometry permitted, through the visual surface brightness relation, high-quality angular-diameter values for each Cepheid throughout its pulsation. The simultaneous radial velocities permitted the linear displacement curve to be phase-locked to the angular diameter variation. The results are individual distances and radii with considerably smaller uncertainty than could be obtained previously.

Type
Part I. Fundamental Parameters
Copyright
Copyright © Cambridge University Press 1985

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