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Photometric Observations of Three Double Stars by the Occultation Method — Comparison with Interferometric Results and with Preliminary Results of HIPPARCOS
Published online by Cambridge University Press: 12 April 2016
Abstract
We first briefly recall the geometry of the occultation of a double star by the Moon’s edge. Then we give a short description of the principle of the formation of the diffraction pattern. We present the results for three double stars and compare them with those obtained by other methods.
- Type
- High Resolution At Visual Wavelengths
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- Copyright © Astronomical Society of the Pacific 1992