Charge exchange emission and cold clumps in multi-phase galactic outflows
Kinwah Wu, Kaye Jiale Li, Ellis R. Owen, Li Ji, Shuinai Zhang,, Graziella Branduardi-Raymont

TL;DR
This paper investigates the structure and evolution of cold dense clumps in galactic outflows, revealing their flattened shapes, their interaction with ionised fluid, and their role in galactic material recycling.
Contribution
It provides observational evidence and analysis of cold clump morphology and dynamics in galactic outflows, supporting models of clump compression, ablation, and recycling.
Findings
Cold dense clumps are flattened, pancake-like structures.
Filamentary features are stripped material, not original clumps.
Some clumps survive and seed circumgalactic medium.
Abstract
Large-scale outflows from starburst galaxies are multi-phase, multi-component fluids. Charge-exchange lines which originate from the interfacing surface between the neutral and ionised components are a useful diagnostic of the cold dense structures in the galactic outflow. From the charge-exchange lines observed in the nearby starburst galaxy M82, we conduct surface-to-volume analyses and deduce that the cold dense clumps in its galactic outflow have flattened shapes, resembling a hamburger or a pancake morphology rather than elongated shapes. The observed filamentary H features are therefore not prime charge-exchange line emitters. They are stripped material torn from the slow moving dense clumps by the faster moving ionised fluid which are subsequently warmed and stretched into elongated shapes. Our findings are consistent with numerical simulations which have shown that cold…
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