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1998•arXiv (Cornell University)Open access

The LMC distance modulus from Hipparcos RR Lyrae and classical Cepheid data

X. Luri, A. E. Gómez, J. Torra, F. Figueras, M. O. Mennessier

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Abstract

The LM method, designed to exploit the Hipparcos data to obtain luminosity calibrations, is applied to derive luminosity calibrations for RR Lyrae and classical Cepheids. From these calibrations the distance to the Large Magellanic Cloud (LMC) is estimated. The distance moduli provided by the two calibrations are in good agreement, giving a value of 18.3m, while several previous calibrations using Hipparcos data provided inconsistent results between both types of stars. This result suggests that the Hubble constant should have a value of H_0 = 79 km s-1 Mpc-1.

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What this paper is about

The LM method, designed to exploit the Hipparcos data to obtain luminosity calibrations, is applied to derive luminosity calibrations for RR Lyrae and classical Cepheids. From these calibrations the distance to the Large Magellanic Cloud (LMC) is estimated. The distance moduli provided by the two calibrations are in good agreement, giving a value of 18.3m, while several previous calibrations using Hipparcos data provided inconsistent results between both types of stars. This result suggests that the Hubble constant should have a value of H_0 = 79 km s-1 Mpc-1.

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Available abstract

The LM method, designed to exploit the Hipparcos data to obtain luminosity calibrations, is applied to derive luminosity calibrations for RR Lyrae and classical Cepheids. From these calibrations the distance to the Large Magellanic Cloud (LMC) is estimated. The distance moduli provided by the two calibrations are in good agreement, giving a value of 18.3m, while several previous calibrations using Hipparcos data provided inconsistent results between both types of stars. This result suggests that the Hubble constant should have a value of H_0 = 79 km s-1 Mpc-1.

Key concepts: Cepheid variable, RR Lyrae variable, Distance modulus, Physics, Large Magellanic Cloud, Luminosity, Astrophysics, Hubble's law

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