Precise Empirical Determination of Metallicity Dependence of Near-infrared Period-Luminosity Relations for RR Lyrae Variables
Anupam Bhardwaj, Marcella Marconi, Marina Rejkuba, Richard de Grijs,, Harinder P. Singh, Vittorio F. Braga, Shashi Kanbur, Chow-Choong Ngeow,, Vincenzo Ripepi, Giuseppe Bono, Giulia De Somma, and Massimo Dall'Ora

TL;DR
This study empirically quantifies how metallicity influences near-infrared period-luminosity relations for RR Lyrae stars, improving distance measurement accuracy in astronomy.
Contribution
It provides the first precise empirical determination of the metallicity dependence of NIR PLRs for RR Lyrae variables across a large metallicity range.
Findings
Metallicity dependence of ~0.2 mag/dex in NIR PLZ and PWZ relations.
Empirical relations agree with theoretical models.
RR Lyrae distances are consistent with other methods.
Abstract
RR Lyrae variables are excellent population II distance indicators thanks to their well-defined period-luminosity relations (PLRs) at infrared wavelengths. We present results of near-infrared (NIR) monitoring of Galactic globular clusters to empirically quantify the metallicity dependence of NIR PLRs for RR Lyrae variables. Our sample includes homogeneous, accurate, and precise photometric data for 964 RR Lyrae variables in 11 globular clusters covering a large metallicity range (~dex). We derive band period-luminosity-metallicity (PLZ) and period-Wesenheit-metallicity (PWZ) relations anchored using 346 Milky Way field RR Lyrae stars with {\it Gaia} parallaxes, and simultaneously solved for independent distances to globular clusters. We find a significant metallicity dependence of ~mag/dex in band PLZ and PWZ relations for RR Lyrae…
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Taxonomy
TopicsSpacecraft and Cryogenic Technologies · Inorganic Fluorides and Related Compounds · Solid-state spectroscopy and crystallography
