GASKAP-HI Pilot Survey Science III: An unbiased view of cold gas in the Small Magellanic Cloud

Abstract

We present the first unbiased survey of neutral hydrogen (HI) absorption in the Small Magellanic Cloud (SMC). The survey utilises pilot HI observations with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope as part of the Galactic ASKAP HI (GASKAP-HI) project whose dataset has been processed with the GASKAP-HI absorption pipeline, also described here. This dataset provides absorption spectra towards 229 continuum sources, a 275% increase in the number of continuum sources previously published in the SMC region, as well as an improvement in the quality of absorption spectra over previous surveys of the SMC. Our unbiased view, combined with the closely matched beam size between emission and absorption, reveals a lower cold gas faction (11%) than the 2019 ATCA survey of the SMC and is more representative of the SMC as a whole. We also find that the optical depth varies greatly between the SMC's bar and wing regions. In the bar we find that the optical depth is generally low (correction factor to the optically thin column density assumption of ${\mathcal{R}}_{\mathrm{HI}}\sim 1.04$) but increases linearly with column density. In the wing however, there is a wide scatter in optical depth despite a tighter range of column densities.

Accepted for publication in PASA, 19 pages, 17 figures, 5 tables

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• The Atomic to Molecular Transition in Galaxies. II: HI and H_2 Column Densities
• GASS: The Parkes Galactic All-Sky Survey. Update: improved correction for instrumental effects and new data release
• The 21-SPONGE HI Absorption Survey I: Techniques and Initial Results
• Cold and warm atomic gas around the Perseus molecular cloud I: Basic Properties
• GASKAP-HI Pilot Survey Science III: An unbiased view of cold gas in the Small Magellanic Cloud
• Cold HI ejected into the Magellanic Stream
• The MACH HI absorption survey I: Physical conditions of cold atomic gas outside of the Galactic plane

Cited by in corpus (6)

• GASKAP-HI Pilot Survey Science III: An unbiased view of cold gas in the Small Magellanic Cloud
• A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
• Probing the cold neutral medium through HI emission morphology with the scattering transform
• A neutral hydrogen absorption study of cold gas in the outskirts of the Magellanic Clouds using the GASKAP-HI survey
• Considerations with stacking absorption spectra: cold HI gas in cirrus region of the Milky Way
• Processing of GASKAP-HI pilot survey data using a commercial supercomputer