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Paper: Cool Stars in Wide Binaries: 23,000 Common Proper Motion Doubles from the SUPERBLINK Proper Motion Survey
Volume: 448, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Page: 1375
Authors: Lépine, S.
Abstract: The current version of the SUPERBLINK proper motion catalog, now listing over 2,800,000 stars with proper motions μ > 40 mas/yr, is searched for common proper motion pairs. Statistical analysis demonstrates that the catalog already contains more than 18,000 co-moving pairs which are most likely to be wide binaries. Many of these are relatively nearby (d< 100 pc) low-mass systems with K and M dwarf components. However, we also identify about 1,200 high-velocity systems, whose components are mostly old, metal-poor K and M subdwarfs associated with the Galactic thick disc or halo. We estimate that the field population has a wide-binary multiplicity fraction of at least 1.3% for low-mass stars (K–M dwarfs), while the local old population has a multiplicity fraction of at least 0.43% (K–M subdwarfs).
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