Authors: Jeffrey Joseph Wolynski
In the recent paper, “KELT-17b: A Hot-Jupiter Transiting an A-Star in a Misaligned Orbit Detected with Doppler Tomography”, it is referenced that, “a sample of well characterized planets around massive stars is necessary to understand the mass-dependence of planet properties.” Two principles are provided to explain that mass-dependence attributed to formation processes is moot. Explanation is provided.
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[v1] 2016-07-16 14:37:29
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