Image Details
Caption: Figure 4.
Posterior distributions for orbital parameters of a possible circumbinary companion around J2043+1711. The orbital period and companion mass are well constrained by the model, although the configuration of the orbit can only be constrained to lie within a specific quadrant. The inclination angle of the orbit is not constrained, and is strongly covariant with the orbital period.
© 2025. The Author(s). Published by the American Astronomical Society.