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- W4236722141 abstract "Long-baseline optical interferometry has made it possible to measure the visual orbits of binary stars with major axes as small as 5 mas and errors of ≲ 100 μas. Interferometers now nearing completion will extend these values to ≳ 500 μas and σ a ∼ 10 μas. Observations of double-lined spectroscopic binaries with current interferometers have already yielded some mass estimates with precisions rivaling those from fitting the light curves of eclipsing double-lined systems. Luminosity estimates based on combined visual interferometric observations and velocity curves are often more precise than those from more indirect methods based on estimates of T eff . New interferometers now coming into operation will make it possible to measure fundamental parameters in dozens to hundreds of binary systems." @default.
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- W4236722141 date "1995-01-01" @default.
- W4236722141 modified "2023-10-18" @default.
- W4236722141 title "Sub-Milliarcsecond Optical Astrometry and Binary Stars" @default.
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- W4236722141 doi "https://doi.org/10.1017/s0074180900228064" @default.
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