Optical Interferometry: Some Current Results and How They Grew

Details Optical Interferometry: Some Current Results and How They Grew Optical Interferometry: Some Current Results and How They Grew

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.8601a&link_type=abstract

American Astronomical Society Meeting 207, #86.01; Bulletin of the American Astronomical Society, Vol. 37, p.1312

Astronomy and Astrophysics

Astronomy

Scientific paper

In the first part of the 20th century, optical interferometers produced diameter measurements for a few bright stars and orbits for a few binaries. The last decade has brought new arrays and improved techniques. With these improvements has come a wider range of results, including limb darkening, orbits of triple systems, Cepheid pulsations, shapes of rapid rotators, images of circumstellar material, high-precision astrometry, and even detection of AGNs. I will introduce some of the current directions in optical interferometry and how the increased capabilities of current instruments have made them possible.

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