New absolute magnitude calibrations for W Ursa Majoris type binaries
Z. Eker, S. Bilir, E. Yaz, O. Demircan, M. Helvaci

TL;DR
This paper recalibrates the Period-Luminosity-Color relation for W UMa stars using Hipparcos parallaxes, providing improved distance estimates and an infrared-based calibration despite single-epoch data limitations.
Contribution
It introduces new absolute magnitude calibrations for W UMa stars, including an infrared relation, based on bias-corrected parallaxes and extensive data analysis.
Findings
Revised PLC relation closely matches previous for nearby stars.
Infrared PLC relation is reliable despite single-epoch 2MASS data.
Bias correction significantly impacts distance estimates at larger distances.
Abstract
Parallaxes of W UMa stars in the Hipparcos catalogue have been analyzed. 31 W UMa stars, which have the most accurate parallaxes () which are neither associated with a photometric tertiary nor with evidence of a visual companion, were selected for re-calibrating the Period--Luminosity--Color (PLC) relation of W UMa stars. Using the Lutz--Kelker (LK) bias corrected (most probable) parallaxes, periods (), and colors (0.04<<1.28) of the 31 selected W UMa, the PLC relation have been revised and re-calibrated. The difference between the old (revised but not bias corrected) and the new (LK bias corrected) relations are almost negligible in predicting the distances of W UMa stars up to about 100 parsecs. But, it increases and may become intolerable as distances of stars increase. Additionally, using and colors…
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