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Absolute Properties of the Highly Eccentric, Solar-type Eclipsing Binary HD 74057

  • Authors: James R. Sowell, Gregory W. Henry, and Francis C. Fekel

Sowell, Henry, & Fekel 2012 The Astronomical Journal 143 5.

  • Provider: AAS Journals

Caption: Figure 7.

Positions of the two components of HD 74057 (primary: filled circle; secondary: open circle) in a theoretical H-R diagram compared with the Yonsei-Yale evolutionary tracks. The dashed line corresponds to a track for the mean mass of the components ( M = 1.134 M ) and solar metallicity, while the solid line results from the same mass but a metallicity of Z = 0.031 or [Fe/H] = 0.2.

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