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No Giant Planets in the Eta Cassiopeiae System: Dynamical Implications of a Wide Binary Companion

  • Authors: Stephen R. Kane, Zhexing Li, Michelle L. Hill, Skylar D'Angiolillo, Benjamin J. Fulton, Andrew W. Howard

Stephen R. Kane et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 4.

Results of the dynamical simulation for the Eta Cas system as a function of semimajor axis of the injected planet. The top panel provides the percentage survival calculations for the planet, and the bottom panel shows the maximum eccentricity of the planet. The extent of the HZ is shown in green, where the light green and dark green regions indicate the CHZ and OHZ, respectively.

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