Image Details

Choose export citation format:

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 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.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse