Image Details
Caption: Figure 3.
Histogram of 72 primary M dwarfs with astrometry from ground-based efforts by the RECONS team, the Yale Parallax Catalog, or from other sources in the literature, plotted in equal-volume shells with increasing distance from the Sun. Most of these M dwarf systems are well within 25 pc and likely to remain in RMSTAR after more precise parallaxes are determined in future Gaia data releases.
© 2026. The Author(s). Published by the American Astronomical Society.