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Near-Surface Constraints on the Structure of Stellar Convection Zones
1997By simulating the convection in the upper layers of six different stars and matching these simulations to 1D-mixing length models using the same input physics, we have been able to infer the behaviour of the mixing-length parameter, α, as the stellar parameters changes.
Trampedach, Regner +3 more
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Studies on Stellar Models with Partially Degenerate Cores and Outer Convective Zones
Publications of the Astronomical Society of Japan, 1958Abstract Stellar models with partially degenerate isothermal cores and outer convective zones have been investigated taking account of the contribution of the ion pressure in the core. All models have been computed for two different contents of the heavy elements.
Mahiro Shimoda, Shinya Obi
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Penetrative convection in rotating fluids: A model for the base of stellar convection zones
Geophysical & Astrophysical Fluid Dynamics, 1991Abstract To model penetrative convection at the base of a stellar convection zone we consider two plane parallel, co-rotating Boussinesq layers coupled at their fluid interface. The system is such that the upper layer is unstable to convection while the lower is stable.
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Integrative oncology: Addressing the global challenges of cancer prevention and treatment
Ca-A Cancer Journal for Clinicians, 2022Jun J Mao,, Msce +2 more
exaly
A convective model for turbulent mixing in rotating convection zones. [in stellar dynamics]
, 1984D. Hathaway
semanticscholar +1 more source
Wave generation and pulsation in stars with convective zones
, 1977W. Unno
semanticscholar +1 more source
Multidisciplinary standards of care and recent progress in pancreatic ductal adenocarcinoma
Ca-A Cancer Journal for Clinicians, 2020Aaron J Grossberg +2 more
exaly