http://arxiv.org/abs/1506.06344
The so-called “global polytropic model” is applied to the numerical study of the exoplanet systems HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186. We compare computed distances of planets from their host stars with corresponding observations and discuss some further orbit predictions made by the model.
V. Geroyannis
Tue, 23 Jun 15
66/67
Comments: 10 pages
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