Add to ORKGThe Infrared Spatial Interferometer (ISI) has been conducting mid-IR measurements of red supergiant and AGB stars for about 20 years. This paper reviews the ISI system and results with an emphasis on measurements of changes in stellar sizes and shapes, and those of the surrounding dust shells, over time scales of weeks to decades. The long-term measurement record provides important new observables for stellar theory. A new spectrometer-correlator system is discussed where this system will measure visibilities on-and-off individual molecular spectral lines
We have conducted the first systematic study of Herbig Ae/Be stars using the technique of long basel...
Recent years have seen a major contribution of infrared interferometry to studies on the circumste...
We present the first long baseline mid-infrared interferometric observations of the circumstell...
The Infrared Spatial Interferometer (ISI) is a three telescope interferometer system that operates n...
The Infrared Spatial Interferometer (ISI) has been conducting mid-infrared observations of late-type...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
Over the past twenty years the U. C. Berkeley Infrared Spatial Interferometer has observed a number ...
Infrared interferometric demonstrations with the University of California, Berkeley's infrared spati...
element stellar interferometer which employs heterodyne detection to gather starlight in the mid-inf...
The dynamics of the surface and inner atmosphere of the red supergiant star Betelgeuse are the subje...
The structure and composition of circumstellar disks around young stars is one of the areas in which...
Since 1975 McCarthy and Low have conducted a program of Michelson spatial interferometry at infrared...
Infrared interferometry promises to be a useful astrometric technique. Preliminary measurements of t...
Red supergiants (RSGs) are cool, luminous stars with radii that can exceed 1000 R⊙. Indeed, such is ...
The results of a high-resolution interferometric campaign targeting the symbiotic long-period variab...
We have conducted the first systematic study of Herbig Ae/Be stars using the technique of long basel...
Recent years have seen a major contribution of infrared interferometry to studies on the circumste...
We present the first long baseline mid-infrared interferometric observations of the circumstell...
The Infrared Spatial Interferometer (ISI) is a three telescope interferometer system that operates n...
The Infrared Spatial Interferometer (ISI) has been conducting mid-infrared observations of late-type...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
Over the past twenty years the U. C. Berkeley Infrared Spatial Interferometer has observed a number ...
Infrared interferometric demonstrations with the University of California, Berkeley's infrared spati...
element stellar interferometer which employs heterodyne detection to gather starlight in the mid-inf...
The dynamics of the surface and inner atmosphere of the red supergiant star Betelgeuse are the subje...
The structure and composition of circumstellar disks around young stars is one of the areas in which...
Since 1975 McCarthy and Low have conducted a program of Michelson spatial interferometry at infrared...
Infrared interferometry promises to be a useful astrometric technique. Preliminary measurements of t...
Red supergiants (RSGs) are cool, luminous stars with radii that can exceed 1000 R⊙. Indeed, such is ...
The results of a high-resolution interferometric campaign targeting the symbiotic long-period variab...
We have conducted the first systematic study of Herbig Ae/Be stars using the technique of long basel...
Recent years have seen a major contribution of infrared interferometry to studies on the circumste...
We present the first long baseline mid-infrared interferometric observations of the circumstell...