Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996auja....6..175d&link_type=abstract
Aust. J. Astron., Vol. 6, Nos. 5 - 6, p. 175 - 179
Astronomy and Astrophysics
Astronomy
Stellar Interferometers: Stellar Diameters, Effective Temperatures: Stellar Interferometers, Effective Temperatures: Spectrophotometry
Scientific paper
The Sydney University Stellar Interferometer (SUSI) is a new optical instrument designed to measure the angular diameters of stars and the angular separations of close binary stars. The angular dimensions, in combination with complementary photometry, spectrophotometry, and spectroscopy, enable fundamental properties of stars to be determined. A specific example is the combination of angular diameters with observed spectral flux distributions to determine emergent flux distributions and effective temperatures. The potential accuracy of empirical determinations of effective temperature as a function of spectral type is discussed.
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