Published May 21, 2025 | Version v1
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MINDS. Water reservoirs of compact planet-forming dust disks: A diversity of H2O distributions

Description

This repository contains the appendix figure of the paper: "MINDS: Water reservoirs of compact planet-forming dust disks: A diversity of H2O distributions".
The figures are numbered based on how they appeared in the initial arxiv version (2505.15237, after the paper has been accepted for publication in Astronomy & Astrophysics). 

The table below contains the caption for each figure:

File name Appendix figure Caption
BPTau-BestProfile.png D.2 Comparison between the full models of the best-fitting parametric model (bottom fit) and of the multiple components (red, top fit) for BP Tau. The colour of the best-fitting profile matches that of Figure 3. Indicated are also the molecular features from OH (magenta), CO2 (green), and HCN (orange). The vertical lines indicate the S(1) and S(2) transitions of H2.
CXTau-BestProfile.png D.3 Similar as Figure D.2, but for CX Tau. We refer the reader to Vlasblom et al. (2024b) for the other molecular emission features.
CYTau-BestProfile.png D.4 Similar as Figure D.2, but for CY Tau. Highlighted in yellow is the C2H2 emission feature, while the approximate location of 13-CCH2 is also shown.
DNTau-BestProfile.png D.5 Similar as Figure D.2, but for DN Tau. The boxes indicate the detection of 13-CO2 and the potential detection of CO-18-O.
DRTau-BestProfile.png D.6 Similar as Figure D.2, but for DR~Tau. We refer the reader to Temmink et al. (2024a) and Temmink et al. (2024b) for the other molecular emission features.
FTTau-BestProfile.png D.7 Similar as Figure D.2, but for FT Tau. Highlighted in yellow is the C2H2 emission feature.
RNO90-BestProfile.png D.8 Similar as Figure D.2, but for RNO 90. Highlighted in yellow is the C2H2 emission feature.
XXCha-BestProfile.png D.9 Similar as Figure D.2, but for XX Cha. Highlighted in yellow is the C2H2 emission feature.

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Is supplement to
Journal article: arXiv:2505.15237 (arXiv)