Visible and near-infrared spectro-interferometric analysis of the edge-on Be star o Aquarii

@article{Almeida2020VisibleAN,
  title={Visible and near-infrared spectro-interferometric analysis of the edge-on Be star o Aquarii},
  author={E. S. G. de Almeida and Anthony Meilland and A. Domiciano de Souza and P. Stee and Denis Mourard and Nicolas Nardetto and Roxanne Ligi and I. Tallon-Bosc and Daniel Moser Faes and Alex C. Carciofi and Daniel Bednarski and B. C. Mota and Neal J. Turner and Theo A. ten Brummelaar},
  journal={Astronomy and Astrophysics},
  year={2020},
  volume={636}
}
We present a detailed visible and near-IR spectro-interferometric analysis of the Be-shell star $\omicron$ Aquarii from quasi-contemporaneous CHARA/VEGA and VLTI/AMBER observations. We measured the stellar radius of $\omicron$ Aquarii as 4.0 $\pm$ 0.3 $\mathrm{R_{\odot}}$. We constrained the disk geometry and kinematics using a kinematic model and a MCMC fitting procedure. The disk sizes in H$\alpha$ and Br$\gamma$ were found to be similar, at $\sim$10-12 $\mathrm{D_{\star}}$, which is uncommon… 
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