Radii and Distances of Cepheids. I. Method and Measurement Errors
- 20 April 1997
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 479 (2) , 875-885
- https://doi.org/10.1086/303892
Abstract
We develop a formulation of the Baade-Wesselink method which uses the Fourier coefficients of the observables. We derive an explicit, analytic expression to determine the mean radius from each Fourier order. The simplicity of this method allows us to derive the uncertainty in the mean radius due to measurement errors. Using simulations and a recent dataset we demonstrate that the precision of the radius measurement with optical magnitudes is in most cases limited by the accuracy of the measurement of the phase difference between the light and the color index curve. In this case it is advantageous to determine the inverse radius, because it has normal errorsKeywords
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This publication has 10 references indexed in Scilit:
- On Spectral Line Formation and Measurement in Cepheids: Implications to Distance DeterminationThe Astrophysical Journal, 1995
- The radii of Galactic CepheidsMonthly Notices of the Royal Astronomical Society, 1995
- Near-infrared variant of the Barnes-Evans method for finding Cepheid distances calibrated with high-precision angular diametersThe Astronomical Journal, 1994
- The Cepheid Period-Luminosity Relation from Independent Distances of 100 Galactic VariablesThe Astrophysical Journal, 1993
- The period-radius relation for classical Cepheids from the visual surface brightness techniqueThe Astrophysical Journal, 1989
- On the Baade-Wesselink methodVistas in Astronomy, 1987
- The effect of radial and non-radial stellar oscillations on the light, colour and velocity variationsMonthly Notices of the Royal Astronomical Society, 1979
- Application of the Method of Maximum Likelihood to the Determination of Cepheid RadiiMonthly Notices of the Royal Astronomical Society, 1977
- The Conversion Factor from Radial to Pulsational Velocity and the Radii of Classical CepheidsThe Astrophysical Journal, 1972
- Über eine Möglichkeit, die Pulsationstheorie der δ Cephei‐Veränderlichen zu prüfenAstronomische Nachrichten, 1926