Image Details
Caption: Figure 2.
MG vs. ﹩{M}_{{H}_{P}}﹩ for K dwarfs in RKSTAR (orange) and M dwarfs in RMSTAR (dark red). A linear fit, shown in black, is used to convert MHp to MG to define Hipparcos boundaries for K and M dwarfs.
© 2026. The Author(s). Published by the American Astronomical Society.