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Binary star astronomy with optical interferometry

Pan, Xiaopei and Shao, Michael and Colavita, M. Mark (1994) Binary star astronomy with optical interferometry. In: Amplitude and Intensity Spatial Interferometry II. Proceedings of SPIE. No.2200. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, pp. 360-371. ISBN 0-8194-1495-6. https://resolver.caltech.edu/CaltechAUTHORS:20170918-140319236

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Abstract

The Mark III Interferometer on Mt. Wilson, a long-baseline optical interferometer, was in daily operation for more that seven years. During that time it achieved milliarcsecond angular resolution for binary star astronomy, with submilliarcsecond accuracy. For the first time many spectroscopic binaries have been resolved, including binaries in which the companion cannot be detected with spectroscopy. The high angular resolution means that the traditional gap between visual and spectroscopic binaries has been decreased by more than an order of magnitude. In order to confirm the performance of the Mark III Interferometer, this paper uses the results of astronomical observations, and compares the Mark III Interferometer with other high-resolution techniques, including astrometry, lunar occultation, photometry, speckle, and spectroscopy. Comparisons for a variety of binary stars among these techniques indicate that long baseline optical interferometry proves a reliable, fully automatic, daily accessible astronomical capability for achieving high resolution, high accuracy, high dynamic range, and high photometric measurement precision for the study of binary stars.


Item Type:Book Section
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http://dx.doi.org/10.1117/12.177253DOIArticle
https://www.spiedigitallibrary.org/conference-proceedings-of-spie/2200/1/Binary-star-astronomy-with-optical-interferometry/10.1117/12.177253.fullPublisherArticle
Additional Information:© 1994 Society of Photo-Optical Instrumentation Engineers (SPIE). 9 June 1994. The authors are grateful for financial support from the National Aeronautics and Space Administration. Thanks to the people of the interferometric group at NRL and USNO for the observation time, and to Lu Rarogiewicz for assistance in observation. Literature survey is based on the SIMBAD data retrieval system, data base of the Strasbourg, France, Astronomical Data Center.
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Series Name:Proceedings of SPIE
Issue or Number:2200
Record Number:CaltechAUTHORS:20170918-140319236
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170918-140319236
Official Citation:Xiaopei Pan, Michael Shao, M. Mark Colavita, "Binary star astronomy with optical interferometry", Proc. SPIE 2200, Amplitude and Intensity Spatial Interferometry II, (9 June 1994); http://dx.doi.org/10.1117/12.177253
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:81535
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:19 Sep 2017 16:55
Last Modified:03 Oct 2019 18:44

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