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astro-ph.GA2026
The impact of the turbulent Mach number on star formation and the initial mass function
Sajay Sunny Mathew, Christoph Federrath, Amit Seta
Turbulence regulates star formation by influencing the density structure and fragmentation of molecular clouds, and therefore it is expected to play a key role in setting the initi…
astro-ph.GA2025
Study of HI Turbulence in the SMC Using Multi-point Structure Functions
Bumhyun Lee, Min-Young Lee, Jungyeon Cho +19
Turbulence in the interstellar medium (ISM) plays an important role in many physical processes, including forming stars and shaping complex ISM structures. In this work, we investi…
astro-ph.GA2024
Magnetised HI superbubbles in the Small Magellanic Cloud revealed by the POSSUM pilot survey
Seoyoung Lyla Jung, A. Seta, J. M. Price +13
Neutral hydrogen (HI) bubbles and shells are common in the interstellar medium (ISM). Studying their properties provides insight into the characteristics of the local ISM as well a…