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Rotation & Spots with the VLTI: Practice Session

Published online by Cambridge University Press:  10 September 2015

A. Domiciano deSouza
A. Domiciano deSouza*
Affiliation:
Laboratoire J.-L. Lagrange, UMR 7293, Observatoire de la Côte d'Azur (OCA), Université de Nice-Sophia Antipolis (UNS), Centre National de la Recherche Scientifique (CNRS), Campus Valrose, 06108 Nice Cedex 2, France
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Abstract

We present here two examples of the use of interferometric observations to study stellar rotation effects (flattening and gravity darkening) and spots on the stellar photospheres. From the fit of simple geometrical models to two sets of VLTI data (VINCI and AMBER) using the LITpro tool from JMMC we can estimate stellar physical parameters and have insights on the photospheric intensity distribution.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 70: What the Highest Angular Resolution Can Bring to Stellar Astrophysics? , 2014 , pp. 309 - 316
Copyright
© EAS, EDP Sciences, 2015

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References

Domiciano de Souza, A., Vakili, F., Jankov, S., Janot-Pacheco, E., & Abe, L., 2002, A&A, 393, 345
Domiciano de Souza, A., Kervella, P., Jankov, S., et al., 2003, A&A, 407, L47
Domiciano de Souza, A., Bendjoya, P., Vakili, F., Millour, F., & Petrov, R.G., 2008, A&A, 489, L5
Espinosa Lara, F., & Rieutord, M., 2011, A&A, 533, A43
Kervella, P., & Domiciano de Souza, A., 2006, A&A, 453, 1059