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The Rotation Period of the Planet-Hosting Star HD 189733

  • Authors: Gregory W. Henry and Joshua N. Winn

HENRY & WINN 2008 The Astronomical Journal 135 68.

  • Provider: AAS Journals

Caption: Figure 1.

Photometric variability of HD 189733, as observed with the T10 0.8 m APT in the ( b + y)/2 passband. The magnitude difference between HD 189733 and the comparison star HD 189410 is plotted. The top panel shows the entire data set, while the other panels focus on each of the four segments of near-nightly observations.

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