42 citations · 94 across the 4 of their papers we have counts for
4 papers
A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
Isabella A. Gerrard, Christoph Federrath, Nickolas M. Pingel +12
Turbulence plays a crucial role in shaping the structure of the interstellar medium. The ratio of the three-dimensional density contrast () to the turbulent sonic Mach n…
HI filaments as potential compass needles? Comparing the magnetic field structure of the Small Magellanic Cloud to the orientation of GASKAP-HI filaments
Y. K. Ma, N. M. McClure-Griffiths, S. E. Clark +12
High-spatial-resolution HI observations have led to the realisation that the nearby (within few hundreds of parsecs) Galactic atomic filamentary structures are aligned with the amb…
GASKAP-HI Pilot Survey Science I: ASKAP Zoom Observations of HI Emission in the Small Magellanic Cloud
N. M. Pingel, J. Dempsey, N. M. McClure-Griffiths +53
We present the most sensitive and detailed view of the neutral hydrogen (HI) emission associated with the Small Magellanic Cloud (SMC), through the combination of data from the Aus…
A Radio Polarisation Study of Magnetic Fields in the Small Magellanic Cloud
J. D. Livingston, N. M. McClure-Griffiths, S. A. Mao +4
Observing the magnetic fields of low-mass interacting galaxies tells us how they have evolved over cosmic time and their importance in galaxy evolution. We have measured the Farada…