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arxiv: astro-ph/0406067 · v1 · submitted 2004-06-02 · 🌌 astro-ph

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The RR Lyrae Period-Luminosity Relation. I. Theoretical Calibration

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keywords relationcalibrationperiod-luminositytheoreticaldifferentlyraetypeaccount
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We present a theoretical calibration of the RR Lyrae period-luminosity (PL) relation in the UBVRIJHK Johnsons-Cousins-Glass system. Our theoretical work is based on calculations of synthetic horizontal branches (HBs) for several different metallicities, fully taking into account evolutionary effects besides the effect of chemical composition. Extensive tabulations of our results are provided, including convenient analytical formulae for the calculation of the coefficients of the period-luminosity relation in the different passbands as a function of HB type. We also provide "average" PL relations in IJHK, for applications in cases where the HB type is not known a priori; as well as a new calibration of the M_V - [M/H] relation. These can be summarized as follows: M_I = +0.471 - 1.132 log P + 0.205 log Z, M_J = -0.141 - 1.773 log P + 0.190 log Z, M_H = -0.551 - 2.313 log P + 0.178 log Z, M_K = -0.597 - 2.353 log P + 0.175 log Z, and M_V = +2.288 + 0.882 log Z + 0.108 (log Z)^2.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Photometric metallicity of Galactic RR Lyrae stars in the Gaia DR3 era

    astro-ph.SR 2026-05 conditional novelty 6.0

    A new G-band relation [Fe/H] = -6.93 - 6.04P + 1.65 φ31 calibrated on 72 RR Lyrae stars yields 0.26 dex RMS scatter against spectroscopy.

  2. Photometric metallicity of Galactic RR Lyrae stars in the Gaia DR3 era

    astro-ph.SR 2026-05 unverdicted novelty 6.0

    New G-band relation [Fe/H] = -6.93 - 6.04P + 1.65 φ31 calibrated on 72 RR Lyrae stars with spectroscopic anchors, yielding 0.00 dex bias and 0.26 dex RMS scatter.