Image Details
Caption: Figure 13.
Posterior for the system HIP 389 (Blanco 1-W86), a spectroscopic binary (J. F. González et al. 2024). This shows how the constraints from Gaia RV variability (via the approach from Q. Chance et al. 2025) can provide an orthogonal constraint beyond absolute astrometry.
© 2026. The Author(s). Published by the American Astronomical Society.