Contact Binaries as Viable Distance Indicators: New, Competitive (V)JHKs Period-Luminosity Relations

Abstract

Based on the largest catalogs currently available, comprising 6090 contact binaries (CBs) and 2167 open clusters, we determine the near-infrared $JH{K}_{\mathrm{s}}$ CB period--luminosity (PL) relations, for the first time achieving the low levels of intrinsic scatter that make these relations viable as competitive distance calibrators. To firmly establish our distance calibration on the basis of open cluster CBs, we require that (i) the CB of interest must be located inside the core radius of its host cluster; (ii) the CB's proper motion must be located within the $2\sigma$ distribution of that of its host open cluster; and (iii) the CB's age, $t$, must be comparable to that of its host cluster, i.e., $Δ\log (t\mbox{ yr}^{-1}) <0.3$. We thus select a calibration sample of 66 CBs with either open cluster distances or accurate space-based parallaxes. The resulting near-infrared PL relations, for both late-type (i.e., W Ursae Majoris-type) and---for the first time---early-type CBs, are as accurate as the well-established $JH{K}_{\mathrm{s}}$ Cepheid PL relations, (characterized by single-band statistical uncertainties of $\sigma <0.10$ mag). We show that CBs can be used as viable distance tracers, yielding distances with uncertainties of better than 5\% for 90\% of the 6090 CBs in our full sample. By combining the full $JH{K}_{\mathrm{s}}$ photometric data set, CBs can trace distances with an accuracy, $σ=0.05 \mbox{ (statistical)} \pm0.03 \mbox{ (systematic)}$ mag. The 102 CBs in the Large Magellanic Cloud are used to determine a distance modulus to the galaxy of $(m-M_V{)}_0^{\mathrm{LMC}}=18.41\pm 0.20$ mag.

24 pages, 6 figures, accepted by The Astrophysical Journal

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Cited by in corpus (15)

• The Zwicky Transient Facility Catalog of Periodic Variable Stars
• Statistics of 700 individually studied W UMa stars
• Tidal Synchronization and Differential Rotation of Kepler Eclipsing Binaries
• Binary Stars in the New Millennium
• Gaia EDR3 Parallax Zero-point Offset based on W Ursae Majoris-type Eclipsing Binaries
• The Near-infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-infrared Period--Luminosity Relations
• A Bayesian Analysis of Physical Parameters for 783 Kepler (Near-)Contact Binaries: Extreme-Mass-Ratio Systems and a New Mass Ratio versus Period Lower Limit
• Absolute Magnitude Calibration for W UMa-Type Systems Based on Gaia Data
• Case AD, AR, and AS binary evolution and their possible connections with W UMa binaries
• Eclipsing Binary Populations across the Northern Galactic Plane from the KISOGP survey
• Zwicky Transient Facility and Globular Clusters: the Period-Luminosity and Period-Luminosity-Color Relations for Late-Type Contact Binaries
• A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey
• Astrometric mass measurement of compact companions in binary systems with Gaia
• Period-Luminosity-Metallicity-Color Relations of Late-type Contact Binaries in the Big Data Era
• A hundred new eclipsing binary system candidates studied in a near-infrared window in the VVV survey