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Issue EAS Publications Series
Volume 6, 2003
Observing with the VLTI
Page(s) 273
DOI 10.1051/eas:2003028

Observing with the VLTI
G. Perrin and F. Malbet (eds)
EAS Publications Series, Vol. 6, 2003

DOI: 10.1051/eas:2003028

Interacting binaries and extrasolar planets: Challenges for VLTI

K.D. Gazeas

Department of Astrophysics, Astronomy and Mechanics, Faculty of Physics, University of Athens, GR 157 84, Zografos, Athens, Greece


Abstract
Optical Interferometry can play an important role in modern astronomy. Extrasolar planet and binary star research, are some of the fields, where we will face important discoveries in the future. For the VLTI this will be a real challenge, since it will be the pioneer in angular resolution. In addition, high flux sensitivity will help detecting not only Jupiter-sized planets, but Earth-sized planets too. The ability of the VLTI in detecting new planets, measuring stellar diameters and stellar proper motions, with the use of such techniques, is presented.



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