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SMA 200–400 GHz Survey for 10 Faint Class II Disks in the Taurus Molecular Cloud

  • Authors: Chia-Ying Chung, Hauyu Baobab Liu, Sean M. Andrews, Mark A. Gurwell, Melvyn Wright, Feng Long

Chia-Ying Chung et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

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).

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