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• W2094499466 abstract "We have used the infrared Barnes-Evans surface brightness technique to derive the radii and distances of 34 Galactic Cepheid variables. Radius and distance results obtained from both versions of the technique are in excellent agreement. The radii of 28 variables are used to determine the period-radius (PR) relation. This relation is found to have a smaller dispersion than in previous studies, and is identical to the PR relation found by Laney & Stobie from a completely independent method, a fact which provides persuasive evidence that the Cepheid PR relation is now determined at a very high confidence level. We use the accurate infrared distances to determine period-luminosity (PL) relations in the V, I, J, H, and K passbands from the Galactic sample of Cepheids. We derive improved slopes of these relations from updated LMC Cepheid samples and adopt these slopes to obtain accurate absolute calibrations of the PL relation. By comparing these relations to the ones defined by the LMC Cepheids, we derive strikingly consistent and precise values for the LMC distance modulus in each of the passbands that yield a mean value of μ0(LMC) = 18.46 ± 0.02." @default.
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• W2094499466 date "1998-03-20" @default.
• W2094499466 modified "2023-09-23" @default.
• W2094499466 title "Cepheid Period‐Radius and Period‐Luminosity Relations and the Distance to the Large Magellanic Cloud" @default.
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• W2094499466 doi "https://doi.org/10.1086/305374" @default.
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