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The JDISC Survey: Inner Disk Chemistry of Class I/FS Disks and Tentative Evidence for Early Pebble Drift

  • Authors: Ke Zhang, Andrea Banzatti, Colette Salyk, Abygail Waggoner, Klaus Pontoppidan, María José Colmenares, Ilaria Pascucci, Lucas A. Cieza, Miguel Vioque, Paola Pinilla, Geoffrey A. Blake, Joan Najita, Joe Williams, Sebastiaan Krijt, Till Kaeufer, Jane Huang, Feng Long, Chengyan Xie, Minjae Kim, Eshan Raul, Dary A. Ruíz-Rodríguez, Nicole Arulanantham, Benoît Tabone, Mayank Narang, Karina Mauco

Ke Zhang et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 4.

Line luminosities as a function of accretion luminosity. Top: diagnostic water lines. Bottom: HCN, C2H2, and CO2. The Class I/FS and II samples generally follow the same trends, but Class I/FS shows larger scatter in the water lines. The gray dashed line and shaded band show the censored linmix fit (B. C. Kelly 2007) to the Class II reference sample (16th–84th percentile of the posterior), which includes the upper limits; a separate Class I/FS linmix fit is not shown because too few Class I/FS sources have Lacc detections. The generalized (censored) Kendall τ and its p-value are annotated in each panel for the Class II (τII) and Class I/FS (i < 70; τI) samples, computed separately so the two trends can be compared.

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