Image Details
Caption: Figure 1.
The empirical probability density function p x (x) for the solar-type part of the MS for M67 (blue data points). The red curve with solid red guide points gives a fit of a model probability density function p x (x) to the measured function for M67. The model incorporates a Gaussian width σ = 0.117 and a binary fraction A = 0.353.
© 2026. The Author(s). Published by the American Astronomical Society.