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- W2067167410 abstract "New astrometric–spectroscopic orbital solutions for the single-line K-giant binaries β Reticuli (P≈ 5.2 yr, e= 0.3346 ± 0.0004) and ν Octantis (P≈ 2.9 yr, e= 0.2358 ± 0.0003) have been derived based on high-precision spectroscopic radial velocities (RVs) and the Hipparcos astrometry. For the case of ν Oct, the simultaneous solution is particularly robust and an inclination of i= 70.8 ± 0.9° has been derived. This is one of the most precise inclinations yet calculated based on a spectroscopic solution and the Hipparcos astrometry." @default.
- W2067167410 created "2016-06-24" @default.
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- W2067167410 date "2009-04-11" @default.
- W2067167410 modified "2023-10-18" @default.
- W2067167410 title "Spectroscopic orbits for K giants β Reticuli and ν Octantis: what is causing a low-amplitude radial velocity resonant perturbation in ν Oct?" @default.
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- W2067167410 doi "https://doi.org/10.1111/j.1365-2966.2009.14459.x" @default.
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