Fig. 3 from Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES‐2

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Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES‐2

Authors: Alessandro Sozzetti, Guillermo Torres, David Charbonneau, David W. Latham, Matthew J. Holman, Joshua N. Winn, John B. Laird, and Francis T. O'Donovan

Sozzetti et al. 2007 The Astrophysical Journal 664 1190.

Provider: AAS Journals

Caption: Fig. 3.

Lithium abundance ﹩\mathrm{log}\,\epsilon ﹩ (Li) as a function of effective temperature T_eff for TrES‐2 (filled circle) and a sample of planet hosts (data from Israelian et al. 2004; open circles). Arrows indicate that only upper limits on ﹩\mathrm{log}\,\epsilon ﹩ (Li) are available.

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