Image Details
Caption: Figure 3.
Cumulative distribution functions (CDF) of fitted Gaussian components for selected SMC and LMC sources. Panels (a) through (e) show properties of the CNM components, while panel (f) shows properties of the WNM components. The top row, from left to right, shows the peak optical depth (a), peak velocity (b) and corresponding line width of CNM components (c). The lower panel, from left to right, shows the spin temperature of the CNM (d), and the CNM H I column density (e) and the WNM H I column densities WNM (f) for individual components. We also include the peak optical depth and peak velocity for all of the H I absorption-detected components in the SMC and LMC (dashed lines) as provided by J. Dempsey et al. (2022) and J. Dempsey et al. (2025, in preparation), respectively.
© 2025. The Author(s). Published by the American Astronomical Society.