Ubiquitous velocity fluctuations throughout the molecular interstellar medium
J. D. Henshaw, J. M. D. Kruijssen, S. N. Longmore, M. Riener, A. K., Leroy, E. Rosolowsky, A. Ginsburg, C. Battersby, M. Chevance, S. E. Meidt, S., C. O. Glover, A. Hughes, J. Kainulainen, R. S. Klessen, E. Schinnerer, A., Schruba, H. Beuther, F. Bigiel, G. A. Blanc, E. Emsellem

TL;DR
This study reveals that velocity fluctuations in the interstellar medium occur across all scales and environments, driven by turbulent flows and gravitational instabilities, shaping star-forming gas and galaxy evolution.
Contribution
It provides the first comprehensive measurement of molecular gas motions over a wide spatial range, uncovering oscillatory flows and scale-free turbulence in the ISM.
Findings
Ubiquitous velocity fluctuations across all scales and environments.
Detection of oscillatory gas flows with specific wavelengths.
Identification of turbulence consistent with scale-free fluctuations.
Abstract
The density structure of the interstellar medium (ISM) determines where stars form and release energy, momentum, and heavy elements, driving galaxy evolution. Density variations are seeded and amplified by gas motion, but the exact nature of this motion is unknown across spatial scale and galactic environment. Although dense star-forming gas likely emerges from a combination of instabilities, convergent flows, and turbulence, establishing the precise origin is challenging because it requires quantifying gas motion over many orders of magnitude in spatial scale. Here we measure the motion of molecular gas in the Milky Way and in nearby galaxy NGC 4321, assembling observations that span an unprecedented spatial dynamic range ( pc). We detect ubiquitous velocity fluctuations across all spatial scales and galactic environments. Statistical analysis of these fluctuations…
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