Figure 2 from TTV-determined Masses for Warm Jupiters and Their Close Planetary Companions

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TTV-determined Masses for Warm Jupiters and Their Close Planetary Companions

Authors: Dong-Hong Wu, Songhu Wang, Ji-Lin Zhou, Jason H. Steffen, and Gregory Laughlin

2018 The Astronomical Journal 156 96.

Provider: AAS Journals

Caption: Figure 2.

Orbital architectures of six planetary systems considered in this paper. The sizes of the dots are proportional to the radii of the planets. Planets are colored according to equilibrium temperature ranging from 336 K (purple) to 2219 K (red).

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