From large-scale environment to CGM angular momentum to star forming activities -- I: star-forming galaxies
Sen Wang, Dandan Xu, Shengdong Lu, Zheng Cai, Maosheng Xiang, Shude, Mao, Volker Springel, Lars Hernquist

TL;DR
This paper uses simulations to show how large-scale environments influence the angular momentum of circumgalactic gas, triggering episodic star formation cycles in galaxies.
Contribution
It demonstrates the role of large-scale environment in modulating CGM angular momentum and star formation activity in galaxies, highlighting a pulsating gas motion cycle.
Findings
Large-scale environment triggers episodic star formation.
Circumgalactic gas exhibits synchronized 'breathing' motions.
Galaxy star formation cycles are linked to CGM angular momentum modulations.
Abstract
The connection between halo gas acquisition through the circumgalactic medium (CGM) and galaxy star formation has long been studied. In this series of two papers, we put this interplay within the context of the galaxy environment on large scales (several hundreds of kpc), which, to a certain degree, maps out various paths for galaxy interactions. We use the IllustrisTNG-100 simulation to demonstrate that the large-scale environment modulates the circumgalactic gas angular momentum, resulting in either enhanced (Paper I) or suppressed (Paper II) star formation inside a galaxy. In this paper (Paper I), we show that the large-scale environment around a star-forming galaxy is often responsible for triggering new episodes of star formation. Such an episodic star formation pattern is well synced with a pulsating motion of the circumgalactic gas, which, on the one hand receives angular…
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