activity
20152024
most citedGASKAP-HI Pilot Survey Science I: ASKAP Zoom Observations of HI Emission in the Small Magellanic Cloud

42 citations · 125 across the 10 of their papers we have counts for

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10 papers · 1 filter

astro-ph.GA202423 cited

The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium

V. Pelgrims, N. Mandarakas, R. Skalidis +21

We present the first degree-scale tomography map of the dusty magnetized interstellar medium (ISM) from stellar polarimetry and distance measurements. We used the RoboPol polarimet…

astro-ph.GA202412 cited

On the evolution of the observed Mass-to-Length relationship for star-forming filaments

Jiancheng Feng, Rowan J. Smith, Alvaro Hacar +2

The interstellar medium is threaded by a hierarchy of filaments from large scales (~ 100 pc) to small scales (~ 0.1pc). The masses and lengths of these nested structures may reveal…

astro-ph.GA20239 cited

The Kinematic Structure of Magnetically Aligned HI Filaments

Doyeon Avery Kim, Susan E Clark, Mary E Putman +1

We characterize the kinematic and magnetic properties of HI filaments located in a high Galactic latitude region ( and ). We extra…

astro-ph.GA202320 cited

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…

astro-ph.GA2023

The Atacama Cosmology Telescope: Galactic Dust Structure and the Cosmic PAH Background in Cross-correlation with WISE

Rodrigo Córdova Rosado, Brandon S. Hensley, Susan E. Clark +15

We present a cross-correlation analysis between resolution total intensity and polarization observations from the Atacama Cosmology Telescope (ACT) at 150 and 220 GHz and 15$'…

astro-ph.GA20239 cited

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…