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Planetary Companions to the Metal‐rich Stars BD −10°3166 and HD 52265

  • Authors: R. Paul Butler, Steven S. Vogt, Geoffrey W. Marcy, Debra A. Fischer, Gregory W. Henry, and Kevin Apps

Butler et al. 2000 The Astrophysical Journal 545 504.

  • Provider: AAS Journals

Caption: Fig. 7.

Histogram of metallicities of planet‐bearing stars (solid line), compared to the nearest field stars (dashed line). The majority of the planet‐bearing stars are metal‐rich relative to the Sun, which is itself metal‐rich relative to nearby field stars. The metallicities of the Sun, HD 52265, and BD −10°3166 are indicated from left to right by the tick marks at [Fe/H] = 0.00, 0.11, and 0.50, respectively.

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