activity
20152021
most citedOn the Three-Dimensional Structure of Local Molecular Clouds

94 citations · 433 across the 11 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.GA202031 cited

Resolving the Dust-to-Metals Ratio and CO-to-H Conversion Factor in the Nearby Universe

I-Da Chiang, Karin M. Sandstrom, Jérémy Chastenet +8

We investigate the relationship between the dust-to-metals ratio (D/M) and the local interstellar medium environment at ~2 kpc resolution in five nearby galaxies: IC342, M31, M33,…

astro-ph.GA2020

CHIMPS2: Survey description and CO emission in the Galactic Centre

D. J. Eden, T. J. T. Moore, M. J. Currie +103

The latest generation of Galactic-plane surveys is enhancing our ability to study the effects of galactic environment upon the process of star formation. We present the first data…

astro-ph.GA202020 cited

The turbulent gas structure in the centers of NGC253 and the Milky Way

Nico Krieger, Alberto D. Bolatto, Eric W. Koch +12

We compare molecular gas properties in the starbursting center of NGC253 and the Milky Way Galactic Center (GC) on scales of ~1-100 pc using dendograms and resolution-, area- and n…

astro-ph.GA202070 cited

Ubiquitous velocity fluctuations throughout the molecular interstellar medium

J. D. Henshaw, J. M. D. Kruijssen, S. N. Longmore +23

The density structure of the interstellar medium (ISM) determines where stars form and release energy, momentum, and heavy elements, driving galaxy evolution. Density variations ar…

astro-ph.HE202019 cited

The X-ray Emissivity of Low-Density Stellar Populations

C. O. Heinke, M. G. Ivanov, E. W. Koch +17

The dynamical production of low-mass X-ray binaries and brighter cataclysmic variables (CVs) in dense globular clusters is well-established. We investigate how the X-ray emissivity…

astro-ph.GA202020 cited

Spatial Power Spectra of Dust across the Local Group: No Constraint on Disc Scale Height

Eric W. Koch, I-Da Chiang, Dyas Utomo +4

We analyze the 1D spatial power spectra of dust surface density and mid to far-infrared emission at m in the LMC, SMC, M31, and M33. By forward-modelling the point-sprea…