The SLoWPoKES Catalog of Low-mass Ultra-wide Binaries: A Cool Stars Resource for Testing Fundamental Properties and for Constraining Binary Formation Theory
Saurav Dhital, Andrew A. West, Keivan G. Stassun, Nicholas M. Law

TL;DR
The SLoWPoKES catalog provides a large, diverse sample of low-mass ultra-wide binaries, enabling studies of stellar properties and binary formation mechanisms through follow-up observations and analysis.
Contribution
This work presents the largest catalog of low-mass, ultra-wide binaries, with a new Galactic model for selection and a recalibrated metallicity index, facilitating stellar and formation studies.
Findings
Diverse properties of binary pairs suggest multiple formation modes.
The catalog contains 1342 systems, the largest of its kind.
New metallicity calibration improves abundance measurements.
Abstract
We present results from the Sloan Low-mass Wide Pairs of Kinematically Equivalent Stars (SLoWPoKES) catalog of ultra-wide (10^3-10^5.5 AU), low-mass (K5-M7) common proper motion binaries. We constructed a Galactic model, based on empirical stellar number density and 3D velocity distributions, to select bona fide pairs with probability of chance alignment <5%, making SLoWPoKES an efficient sample for followup observations. Our initial catalog contains 1342 disk dwarf, subdwarf, and white dwarf-red dwarf systems and is the largest collection of low-mass, wide binaries ever assembled. The diversity---in mass, metallicity, age, and evolutionary states---of SLoWPoKES pairs makes it a valuable resource of coeval laboratories to examine and constrain the physical properties of low-mass stars. SLoWPoKES pairs show signatures of two (or more) formation modes in the distribution of the physical…
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