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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 1.

Top: nightly Strömgren Δ y magnitudes from the T10 APT for the 2001–2002 observing season. Middle: frequency spectrum of the Δ y observations showing the best-fit period of 8.49 days, which we take to be the rotation period of the active component(s). Bottom: Δ y observations phased with the 8.49 day rotation period have an amplitude of 0.008 mag. The horizontal dashed lines in the top and bottom panels represent the mean brightness of the Δ y data set.

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