3D simulations find that the convective Urca process reduces mixing efficiency near the convective boundary in a simmering white dwarf but does not restrict the overall size of the convection zone, with the A=23 pair having the largest effect.
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3 Pith papers cite this work. Polarity classification is still indexing.
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3D simulations show the convective Urca process substantially reduces the convection zone size in a simmering white dwarf, though convection extends past the Urca shell.
A parametric avoidance model based on stellar age, metallicity, and multiplicity excludes ~50% of 1.74M Gaia DR3 stars as poor candidates for complex life, retaining 777835 targets and releasing the catalog publicly.
citing papers explorer
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Where Not to Look: A Parametric Avoidance Model for SETI Target Selection
A parametric avoidance model based on stellar age, metallicity, and multiplicity excludes ~50% of 1.74M Gaia DR3 stars as poor candidates for complex life, retaining 777835 targets and releasing the catalog publicly.