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Simulations with new k−ω model offer insights into massive star convection processes
At the boundary between the convective and radiative zones of stars ... lifetime evolution for WNL stars under the same initial conditions, such as mass and metallicity. Additionally, it lowered ...
Nature1mon
Layer cake or plum pudding?
Geochemical observations appeared to support layering, whereas geophysical observations tended to support whole-mantle convection. The potential compositional boundary was typically put at 660 km ...