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Dynamical Mass Demography of Single S-type Planets Shaped by Stellar Companions

  • Authors: Xiumin Huang, Jianghui Ji

Xiumin Huang and Jianghui Ji 2026 The Astrophysical Journal Supplement Series 286 .

  • Provider: AAS Journals

Caption: Figure 2.

The relationship between ΔK for single S-type planets and the period ratio function ﹩{P}_{2}/{P}_{1}^{\frac{1}{3}}﹩. ΔK of systems above the green dashed line could exceed the ESPRESSO observation limit. Solid lines correspond to four different sets of continuous initial conditions with Mp = [0.01, 0.1, 1.0, 10.0] MJup, MA = 1.0 M, MB = 0.5 M, e1 = 0.3, e2 = 0.5, and the mutual inclination imut = 60°. The RV observation baseline Tobs is set to be 30 yr. Among the total 95 confirmed single S-type systems with a2 < 100 au, the primary targets with potentially detected ΔK are marked with triangles, squares, and circles. The magnitude of ΔK for each system decreases sequentially from top to bottom and from left to right, as shown in the upper-right legend.

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