Here I review the current state of the field of optical stellar interferometry, concentrating on
ground-based work although a brief report of space interferometry missions is included. We …

▪ Abstract This review emphasizes the mass loss processes that affect the fates of single
stars with initial masses between one and nine solar masses. Just one epoch of mass loss …

The CHARA Array is a six 1 m telescope optical/IR interferometric array located on Mount
Wilson, California, designed and built by the Center for High Angular Resolution Astronomy …

▪ Abstract The field of optical and infrared (IR) interferometry has seen rapid technical and
scientific progress over the past few years. A number of instruments capable of precise …

We have observed Mira stars with the FLUOR beamcombiner on the IOTA interferometer in
narrow bands around m wavelength. We find systematically larger diameters in bands …

We present first results of an experiment to combine data from Keck aperture masking and
the Infrared-Optical Telescope Array to image the circumstellar environments of evolved …

We present new total intensity and linear polarization VLBA observations of the and maser
transitions of SiO at 42.8 and 43.1 GHz in a number of Mira variable stars over a substantial …

The fibered beam combiner FLUOR, which has provided high accuracy visibility
measurements on the IOTA interferometer, is being moved to the CHARA array which …

The Very Large Telescope Interferometer (VLTI) is a complex system, made of a large
number of separated elements. To prepare an early successful operation, it will require a …

We present K-band interferometric measurements of the limb-darkened (LD) intensity profile
of the M 4 giant star ψ Phoenicis obtained with the Very Large Telescope Interferometer …