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 →
What's new?

Latest publication

Mapping Spatial Variations of H I Turbulent Properties in the Small and Large Magellanic Cloud

Szotkowski, Samuel et al.

Dec. 1, 2019

We developed methods for mapping spatial variations of the spatial power spectrum (SPS) and structure function slopes, with the goal of connecting the statistical properties of neutral hydrogen (H I) with the turbulent drivers. The new methods were applied to the H I observations of the Small and Large Magellanic ...

Read more → | See all publications

Team log-in

Log-in to access the team wiki.

Contact the GASKAP team at gaskap[at]anu.edu.au.

Site design by Marc White, Research School of Astronomy & Astrophysics, Australian National University.
Site & content copyright © 2019, the GASKAP team.
Powered by Django.
Designed with Bootstrap.