3D simulations find that initial disc tilt and binary mass ratio determine preferential accretion onto the primary or secondary star, with polar discs showing the slowest mass loss.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Mean SEDs of z<0.75 quasars redden in MIR/NIR/UV with rising Eddington ratio but blue in optical, showing accretion-rate dependence of Type 1 AGN emission.
A review of protoplanetary disc processes, with emphasis on size sorting as a mechanism that can generate nucleosynthetic isotopic heterogeneities in the Solar System.
citing papers explorer
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Misaligned circumbinary discs around unequal-mass eccentric binaries: alignment, morphology, and binary accretion variability
3D simulations find that initial disc tilt and binary mass ratio determine preferential accretion onto the primary or secondary star, with polar discs showing the slowest mass loss.
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The Dependence of the Mean Spectral Energy Distributions on the Accretion Rate for Quasars with $z < 0.75$ from the Sloan Digital Sky Survey
Mean SEDs of z<0.75 quasars redden in MIR/NIR/UV with rising Eddington ratio but blue in optical, showing accretion-rate dependence of Type 1 AGN emission.
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Dust Processing in Protoplanetary Discs From Infall to Dispersal: the Origin of Solar System Isotopic Heterogeneities
A review of protoplanetary disc processes, with emphasis on size sorting as a mechanism that can generate nucleosynthetic isotopic heterogeneities in the Solar System.