Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
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7 Pith papers cite this work. Polarity classification is still indexing.
7
Pith papers citing it
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astro-ph.GA 7years
2026 7verdicts
UNVERDICTED 7representative citing papers
Stellar surface density independently modulates MgII outflow equivalent width in massive star-forming galaxies at 0.35<z<1.0 observed by DESI.
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.
Void galaxies show modestly higher star formation rates in early spirals and outer disks, lower extinction, and higher gas-fraction proxies than matched galaxies in filaments and walls, suggesting slower quenching in underdense environments.
X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.
NGC 1427A shows a complex star formation history with young (~10 Myr) and intermediate-age (100-300 Myr) clusters that trace environmental processing during its orbit in the Fornax cluster.
Barred galaxies with residual central emission and NUV-r color transition at the bar end represent an intermediate evolutionary phase in bar-driven quenching before full central quenching.
citing papers explorer
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AGN-driven outflows in dwarf galaxies from cosmological simulations: Internal properties and observational signatures
Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
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Stellar Surface Density Modulates MgII Cool-gas Outflow Absorption in DESI Star-forming Galaxies
Stellar surface density independently modulates MgII outflow equivalent width in massive star-forming galaxies at 0.35<z<1.0 observed by DESI.
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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.
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The CAVITY project. The spatially resolved SFR of galaxies in voids
Void galaxies show modestly higher star formation rates in early spirals and outer disks, lower extinction, and higher gas-fraction proxies than matched galaxies in filaments and walls, suggesting slower quenching in underdense environments.
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Investigating central star formation in local AGN host galaxies: is there tension between coeval growth and AGN feedback?
X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.
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The complex history of NGC 1427A revealed by its star clusters and star formation history
NGC 1427A shows a complex star formation history with young (~10 Myr) and intermediate-age (100-300 Myr) clusters that trace environmental processing during its orbit in the Fornax cluster.
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Tracing evolutionary pathways of bar-driven quenching in local Universe disc galaxies
Barred galaxies with residual central emission and NUV-r color transition at the bar end represent an intermediate evolutionary phase in bar-driven quenching before full central quenching.