A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is application/pdf.
Millimeter-Wave Polarization Of Protoplanetary Disks Due To Dust Scattering
2016
Zenodo
Preserved Fulltext
We found a new mechanism of millimeter-wave polarization of protoplanetary disks; the self-scattering. If the dust distribution has anisotropies such as ring or lopsided structure, the thermal emission is scattered by large dust grains to emit polarization at millimeter wavelengths. This will be a new probe of grain growth in protoplanetary disks. We also show an application to HL Tau.
doi:10.5281/zenodo.58382
fatcat:aonayhvixbhlbbhclsncn6x74i