Abstract
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.
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References
Armstrong, J.T., et al.: 1992a, Astron. J., 104 241
Armstrong, J.T., et al.: 1992b, Astron. J., 104 2217
McAlister, H.A. and Hartkopf, W.I.: 1988, CHARA/GSU, 2
Mozurkewich, D., etal: 1991, Astron. J., 101 2207
Pan X.P., et al.: 1990, Astrophys.J., 356 641
Pan X.P., et al.: 1992, Astrophys.J., 384 624
Shao, M., et al.: 1988, Astron. Astrophys., 193 357
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© 1994 Springer Science+Business Media Dordrecht
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Hummel, C.A., Armstrong, J.T. (1994). Mk III Interferometer: Milliarcsecond “Visual” Orbits Of Spectroscopic Binaries. In: Robertson, J.G., Tango, W.J. (eds) Very High Angular Resolution Imaging. International Astronomical Union / Union Astronomique Internationale, vol 158. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0880-5_82
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DOI: https://doi.org/10.1007/978-94-011-0880-5_82
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-2633-5
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