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Radial variations of grain sizes and dust scale heights on the protoplanetary disk of HD 163296
2019
Zenodo
HD 163296 is one of the best examples of the ring and gap structured protoplanetary disks. In addition, this disk is the only target where the ring and gap are spatially resolved in millimeter-wave polarization as well. By performing radiative transfer calculations of self-scattering polarization, we find that grain size and the dust scale height are the key parameters to reproduce the azimuthal and radial distributions of the observed polarization signature. Azimuthal variation in polarization
doi:10.5281/zenodo.3585264
fatcat:tjr2cwuoane7tjr4twm5iasj5y