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A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System

  • Authors: Trifon Trifonov, Anna Wollbold, Martin Kürster, Jan Eberhardt, Stephan Stock, Thomas Henning, Sabine Reffert, R. Paul Butler, Steven S. Vogt, Ansgar Reiners, Man Hoi Lee, Bertram Bitsch, Mathias Zechmeister, Florian Rodler, Volker Perdelwitz, Lev Tal-Or, Jan Rybizki, Paul Heeren, Davide Gandolfi, Oscar Barragán, Olga Zakhozhay, Paula Sarkis, Marcelo Tala Pinto, Diana Kossakowski, Vera Wolthoff, Stefan S. Brems, Vera Maria Passegger

Trifon Trifonov et al 2022 The Astronomical Journal 164 .

  • Provider: AAS Journals

Caption: Figure 4.

Distribution of 1000 randomly sampled NS posteriors integrated for 1 Myr. The black, two-dimensional contours indicate 1, 2, and 3σ confidence intervals of the whole posterior distribution, and the red contours indicate 1, 2, and 3σ confidence intervals for the stable subsample. Only the mean planetary eccentricities and eccentricity amplitudes for all three planets are shown, which are decisive for the system’s stability and dynamical properties. The median values of the total posterior distribution are marked with green lines.

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