Figure 5 from ASTROMETRIC MONITORING OF THE HR 8799 PLANETS: ORBIT CONSTRAINTS FROM SELF-CONSISTENT MEASUREMENTS

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ASTROMETRIC MONITORING OF THE HR 8799 PLANETS: ORBIT CONSTRAINTS FROM SELF-CONSISTENT MEASUREMENTS

Authors: Q. M. Konopacky, C. Marois, B. A. Macintosh, R. Galicher, T. S. Barman, S. A. Metchev, and B. Zuckerman

2016 The Astronomical Journal 152 28.

Provider: AAS Journals

Caption: Figure 5.

Results from our Monte Carlo simulations for HR 8799c. One-dimensional PDFs from all possible solutions are shown for each of the seven free parameters. Solid lines represent unweighted solutions while dashed lines show weighted solutions. All allowed eccentricities have a value of <0.5, and the preferred inclination is 37° ± 12°.

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