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Upper Limits to Long-term Variability of Solar-type Stars from Observations of the Open Cluster M67

  • Authors: Steven R. Spangler

Steven R. Spangler 2026 Research Notes of the AAS 10 .

  • Provider: AAS Journals

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.

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