Simulations match observed outflow masses within 0.5 dex but underpredict velocities by an order of magnitude and show face-on galaxies 15-40% more likely to exhibit detectable outflows than edge-on systems.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Green Pea galaxies show a high companion fraction and ~1 dex density excess in overdense environments, favoring transient starbursts sustained by gas accretion over triggering by close major mergers.
citing papers explorer
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High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
Simulations match observed outflow masses within 0.5 dex but underpredict velocities by an order of magnitude and show face-on galaxies 15-40% more likely to exhibit detectable outflows than edge-on systems.
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Not So Isolated: Green Pea Galaxies in Overdense Environments revealed by VLT/MUSE
Green Pea galaxies show a high companion fraction and ~1 dex density excess in overdense environments, favoring transient starbursts sustained by gas accretion over triggering by close major mergers.