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Mk III Interferometer: Milliarcsecond “Visual” Orbits of Spectroscopic Binaries

Published online by Cambridge University Press:  19 July 2016

C.A. Hummel  and
J.T. Armstrong
C.A. Hummel
Affiliation:
NRL/USNO Optical Interferometer Project, U.S. Naval Observatory - AD 5, 3450 Massachusetts Avenue NW, Washington, DC 20392, USA
J.T. Armstrong
Affiliation:
Universities Space Research Association, Washington, DC, USA

Abstract

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The spectroscopic binary observing program of the Mark III Optical Interferometer has produced four published orbits and 22 preliminary orbits. The mean (formal) precision is 0.3% for measurements of sin i and 0.7% for measurements of the semimajor axis a. We list the stars for which we have obtained orbits or preliminary orbits and describe our data and uncertainty analysis techniques.

Keywords

stars: binaries: spectroscopicstars: binaries: visualtechniques: interferometric
Type
Imaging Results: Optical and Infrared
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 410 - 412
Copyright
Copyright © Kluwer 1994 

References

Armstrong, J.T., et al.: 1992a, Astron. J. 104, 241 CrossRefGoogle Scholar
Armstrong, J.T., et al.: 1992b, Astron. J. 104, 2217 Google Scholar
McAlister, H.A. and Hartkopf, W.I.: 1988, CHARA/GSU 2,Google Scholar
Mozurkewich, D., et al.: 1991, Astron. J. 101, 2207 Google Scholar
Pan, X.P., et al.: 1990, Astrophys. J. 356, 641 Google Scholar
Pan, X.P., et al.: 1992, Astrophys. J. 384, 624 Google Scholar
Shao, M., et al.: 1988, Astron. Astrophys. 193, 357 Google Scholar