Broad parameter study with detailed dust evolution code finds most outer dust traps leaky, producing long-lived O-rich inner discs with C/O < 1, while planetesimal formation is needed for strong blocking.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Wind data over two solar cycles shows the phase lag between A_He and SSN increases monotonically with v_SW; after lag correction, A_He matches at fixed SSN across phases and speeds.
Simulations of turbulent reconnection in relativistic jets show energy-independent acceleration time in the Fermi regime matching theory up to a Larmor radius threshold set by current sheet thickness, then energy-dependent drift regime.
Radial velocity measurements from NIR spectra show one TWA candidate as a spectroscopic binary with 41.9% membership probability and the other as a likely single member with 99.5% probability.
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How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
Broad parameter study with detailed dust evolution code finds most outer dust traps leaky, producing long-lived O-rich inner discs with C/O < 1, while planetesimal formation is needed for strong blocking.
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Helium Variation Across Two Solar Cycles Reveals A Speed-Dependent Phase Lag
Wind data over two solar cycles shows the phase lag between A_He and SSN increases monotonically with v_SW; after lag correction, A_He matches at fixed SSN across phases and speeds.
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Particle Acceleration Time due to Turbulent-Induced Magnetic Reconnection
Simulations of turbulent reconnection in relativistic jets show energy-independent acceleration time in the Fermi regime matching theory up to a Larmor radius threshold set by current sheet thickness, then energy-dependent drift regime.
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Radial Velocities of Low-mass Candidate TWA Members
Radial velocity measurements from NIR spectra show one TWA candidate as a spectroscopic binary with 41.9% membership probability and the other as a likely single member with 99.5% probability.