The Galactic ASKAP (GASKAP) survey is a high spectral resolution study of the HI and OH lines in the Milky Way and Magellanic Systems. Read more →
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Latest publication

H I filaments as potential compass needles? Comparing the magnetic field structure of the Small Magellanic Cloud to the orientation of GASKAP-H I filaments

Ma, Y. K. et al.

May 1, 2023

High-spatial-resolution H I observations have led to the realization that the nearby (within few hundreds of parsecs) Galactic atomic filamentary structures are aligned with the ambient magnetic field. Enabled by the high-quality data from the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope for the Galactic ASKAP H I survey, ...

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