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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 4.

Panels show the median correlation coefficients for each molecular line (labeled to the left of each panel) and different source parameters, with error bars representing one standard deviation. Marker colors map to the color bar representing the correlation coefficient, with positive values in purple and negative values in green. The horizontal axis is labeled by the source parameters tested for correlations, including stellar mass, mass accretion rate, stellar X-ray luminosity, HCO+ flux, H13CO+ flux, 0.9 mm continuum flux, and 13CO flux from left to right.

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