SPH simulations demonstrate viscosity-driven transitions forming NBOL, RAKED, and CENBOL boundary layers in sub-Keplerian flows onto neutron stars, extending TCAF concepts.
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2 Pith papers cite this work. Polarity classification is still indexing.
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J-PLUS DR3 yields Schechter-function stellar mass functions for quiescent and star-forming galaxies at 0.05 <= z <= 0.2 that match prior work, with quiescent galaxies showing higher characteristic mass and flatter faint-end slope.
citing papers explorer
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Timing Properties of Shocked Accretion Flows around Neutron Stars -- II. Viscous Disks and Boundary Layers
SPH simulations demonstrate viscosity-driven transitions forming NBOL, RAKED, and CENBOL boundary layers in sub-Keplerian flows onto neutron stars, extending TCAF concepts.
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J-PLUS: The stellar mass function of quiescent and star-forming galaxies at 0.05 <= z <= 0.2
J-PLUS DR3 yields Schechter-function stellar mass functions for quiescent and star-forming galaxies at 0.05 <= z <= 0.2 that match prior work, with quiescent galaxies showing higher characteristic mass and flatter faint-end slope.