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
Study of HI Turbulence in the SMC Using Multi-point Structure Functions
Lee, Bumhyun et al.
Oct. 1, 2025
Turbulence in the interstellar medium (ISM) plays an important role in many physical processes, including forming stars and shaping complex ISM structures. In this work, we investigate the HI turbulent properties of the Small Magellanic Cloud (SMC) to reveal what physical mechanisms drive the turbulence and at what scales. Using ...
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Contact the GASKAP team at gaskap[at]anu.edu.au.
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