Image Details
Caption: Figure 3.
The 198–358 GHz spectral index (α198−358) versus 337 GHz flux density (F337GHz). The values of F337 GHz have been rescaled to a 140 pc distance, according to the distances of the target sources listed in Table 1. The histograms on the right have been normalized such that the area under each of them is 1.0. We excluded the extended disks, DL Tau, CI Tau, GM Tau, AB Aur, DM Tau, AA Tau, and GO Tau from the sample of C.-Y. Chung et al. (2024).
© 2026. The Author(s). Published by the American Astronomical Society.