Image Details
Caption: Figure 7.
Normalized distributions of velocity separations Δv between adjacent fitted components, shown for all spectra (solid) and split by component count per spectrum: N = 2, N = 3–4, and N ≥ 5. Small Δv dominates, while higher-component spectra show broader tails, indicating richer line-of-sight layering.
© 2026. The Author(s). Published by the American Astronomical Society.