Image Details
Caption: Figure 5.
The NSH equilibrium solutions of the dust and gas velocity. (a, b) The dust (blue) and gas (green) velocity in the radial direction and the azimuthal direction, respectively, as a function of τs. The velocity in the azimuthal direction is relative to the Keplerian velocity vK. Different line styles correspond to different dust-to-gas ratios ϵ. (c, d) The gas velocity relative to the dust in the radial and azimuthal direction, respectively. (e) The resulting polarization angle χ from birdie-like alignment.
© 2026. The Author(s). Published by the American Astronomical Society.