Figure 1 from On the Validity of the “Hill Radius Criterion” for the Ejection of Planets from Stellar Habitable Zones

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On the Validity of the “Hill Radius Criterion” for the Ejection of Planets from Stellar Habitable Zones

Authors: M. Cuntz and K. E. Yeager

CUNTZ & YEAGER 2009 The Astrophysical Journal 697 L86.

Provider: AAS Journals

Caption: Figure 1.

Orbits of the giant planets for the two represented systems, which are HD 188015 (dashed line) and HD 20782 (narrow dotted line). We also give the HZs (gray area) for the two systems. The two HZs are assumed to have identical extents.

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