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Mapping Molecular Ion Distributions in a Diverse Sample of Protoplanetary Disks

  • Authors: Deryl E. Long, L. Ilsedore Cleeves, Charles J. Law, Fred C. Adams, Dana E. Anderson, Sean M. Andrews, Edwin A. Bergin, Jane Huang, A. Meredith Hughes, Chunhua Qi, Kamber R. Schwarz, Jacob B. Simon, David Wilner

Deryl E. Long et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure D1.

Line fluxes vs. source properties: stellar mass, stellar X-ray luminosity, mass accretion rate, 0.9 mm continuum flux, 13CO flux, HCO+ flux, and H13CO+ flux. All fluxes are scaled to a common distance of 160 pc. Marker shapes indicate different source types: filled circles are continuous T Tauris, open circles are transition disks, and stars are Herbigs. Continuum flux values at 0.9 mm were measured from our Band 7 observations and are reported in Table A2. 13CO J = 2−1 flux values were retrieved from K. I. Öberg et al. (2021) for AS 209, GM Aur, HD 163296, and MWC 480, F. Long et al. (2022) for DM Tau and V4046 Sgr, and M. Leemker et al. (2022) for LkCa 15. The black line shows the median fit from linmix and the gray lines show samples from the posterior distribution.

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