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This study explores the data-model variance in disk characteristics around HK Tau A and B using the best-fit model approach. The research sheds light on the differences in the disk structure of the binary stars.
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Data, best-fit model and data–model difference for the disks around HK Tau A and B. ELN Jensen & RAkeson Nature 511, 567-569 (2014) doi:10.1038/nature13521