Simulations with new k−ω model offer insights into massive star convection processes
Nov 21, 2024
Researchers at Yunnan Observatories of the Chinese Academy of Sciences simulated the evolution of massive stars with masses ranging from 50 to 150 solar masses during the nitrogen sequence Wolf-Rayet (WNL) star phase.
https://phys.org/news/2024-11-simulations-insights-massive-star-convection.html
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