The Angular Diameter of $\lambda$ Bo\"{o}tis}

@article{Ciardi2006TheAD,
  title={The Angular Diameter of \$\lambda\$ Bo\"\{o\}tis\}},
  author={David R. Ciardi and Gerard T. van Belle and Andrew F. Boden and Theo A. ten Brummelaar and Harold A. Mcalister and William G. Bagnuolo and Jr. and P. J. Goldfinger and Judit Sturmann and Laszlo Sturmann and N. J. Turner and David H. Berger and R. R. Thompson and Stephen T. Ridgway},
  journal={arXiv: Astrophysics},
  year={2006}
}
Using the CHARA Array and the Palomar Testbed Interferometer, the chemically peculiar star $\lambda$ Bootis has been spatially resolved. We have measured the limb darkened angular diameter to be $\theta_{LD} = 0.533\pm0.029$ mas, corresponding to a linear radius of $R_{\star} = 1.70 \pm 0.10 R_\odot$. The measured angular diameter yields an effective temperature for $\lambda$ Boo of $T_{eff} = 8887 \pm 242$ K. Based upon literature surface gravity estimates spanning $\log{(g)} = 4.0-4.2$ $[\rm… Expand

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