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A Neutral Hydrogen Absorption Study of Cold Gas in the Outskirts of the Magellanic Clouds Using the GASKAP-H I Survey

  • Authors: Hongxing Chen, Snežana Stanimirović, Nickolas M. Pingel, James Dempsey, Frances Buckland-Willis, Susan E. Clark, Helga Dénes, John M. Dickey, Steven Gibson, Katherine Jameson, Ian Kemp, Denis Leahy, Min-Young Lee, Callum Lynn, Yik Ki Ma, N. M. McClure-Griffiths, Claire E. Murray, Hiep Nguyen, Lucero Uscanga, Jacco Th. van Loon, Enrique Vázquez-Semadeni

Hongxing Chen et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 4.

CDF of different properties of our selected sources in the LMC and SMC for all lines of sight (LOSs). The upper left is the total CNM H I column density; the upper right is the total WNM HI column density; the lower left is the total H I column density; and the lower right is the CNM fraction. For comparison, we include data from the 21-SPONGE survey of the Milky Way (C. E. Murray et al. 2018), selecting only LOSs with Galactic latitude ∣b∣ > 30∘ to represent diffuse regions in the Milky Way.

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