Stellar feedback regulates radial gas inflow in the Milky Way center, yielding time-averaged rates that fall from 5e-3 to 1e-6 solar masses per year with both smooth secular and episodic components.
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3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
3D simulations show gas can vault over nuclear rings in barred galaxies via vertical momentum, delivering outer gas to the central region.
Kinetic temperatures in three Galactic Center molecular clouds are revised to 84-95 K using additional formaldehyde lines, indicating combined cosmic-ray and turbulent heating rather than extreme values from prior studies.
citing papers explorer
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Simulations of gas inflow in the Milky Way I. Stellar-Feedback-Regulated Transport from the Central Molecular Zone to the Circumnuclear disk
Stellar feedback regulates radial gas inflow in the Milky Way center, yielding time-averaged rates that fall from 5e-3 to 1e-6 solar masses per year with both smooth secular and episodic components.
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Vaulting the barrier: An intrinsic mechanism to fuel the gas beyond the nuclear ring into the central region of barred galaxies
3D simulations show gas can vault over nuclear rings in barred galaxies via vertical momentum, delivering outer gas to the central region.
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What Heats the Dense Gas in the Galactic Center?
Kinetic temperatures in three Galactic Center molecular clouds are revised to 84-95 K using additional formaldehyde lines, indicating combined cosmic-ray and turbulent heating rather than extreme values from prior studies.