no code implementations • 17 Nov 2020 • J. G. Schulze, Ji Wang, J. A. Johnson, C. T. Unterborn, W. R. Panero
We find that these two measures are unlikely to be resolvable as statistically different unless the bulk density CMF is at least 40% greater than or 50% less than the CMF as inferred from the host star.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics