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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Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.
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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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Higher resolution optical spectra of $M_*<10^{10}~M_{\odot}$ galaxies reveal outflow signatures unresolved by the SDSS
Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.