Abstract
We present a brief review of recent scientific and technical advances at
the Infrared Optical Telescope Array (IOTA). IOTA is a long-baseline
interferometer located atop Mount Hopkins, Arizona. Recent work has
emphasized the use of the three-telescope interferometer completed in
2002. We report on results obtained on a range of scientific targets,
including AGB stars, Herbig AeBe Stars, binary stars, and the recent
outburst of the recurrent nova RS Oph. We report the completion of a new
spectrometer which allows visibility measurements at several high
spectral resolution channels simultaneously. Finally, it is our sad duty
to report that IOTA will be closed this year.
Original language | English |
---|---|
Pages (from-to) | 18 |
Journal | Advances in Stellar Interferometry |
Volume | 6268 |
Publication status | Published - 1 Jul 2006 |