In streaming-instability simulations, gas-dust relative flow becomes azimuthal wherever dust-to-gas ratio exceeds one, so birdie-aligned prolate grains naturally emit the azimuthal polarization seen in disks like HL Tau.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2representative citing papers
Core-scale magnetic fields in star-forming regions are more disordered than cloud-scale fields and align randomly with core orientations and velocity gradients.
citing papers explorer
-
Azimuthal Dust Polarization from Aerodynamically Aligned Grains as Evidence for the Streaming Instability in Protoplanetary Disks
In streaming-instability simulations, gas-dust relative flow becomes azimuthal wherever dust-to-gas ratio exceeds one, so birdie-aligned prolate grains naturally emit the azimuthal polarization seen in disks like HL Tau.
-
Magnetic field alignment with dense cores in the transition between cloud and core scales
Core-scale magnetic fields in star-forming regions are more disordered than cloud-scale fields and align randomly with core orientations and velocity gradients.