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arxiv: 1802.10308 · v1 · pith:5XBB6H4Inew · submitted 2018-02-28 · 🌌 astro-ph.GA

The largely unconstrained multiphase nature of outflows in AGN host galaxies

Claudia Cicone (INAF - OABrera) , Marcella Brusa (University of Bologna) , Cristina Ramos Almeida (Instituto de Astrof\'isica de Canarias) , Giovanni Cresci (INAF-Arcetri) , Bernd Husemann (MPIA) , Vincenzo Mainieri (ESO) This is my paper
classification 🌌 astro-ph.GA
keywords multiphaseoutflowsactiveadvocateconsistentcontaindifferentevolution
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Observations and simulations show that outflows in active galactic nuclei (AGN) contain gas in different phases. To understand their true impact on galaxy evolution, we advocate consistent and unbiased investigation of these multiphase winds in large AGN samples.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068

    astro-ph.GA 2026-06 unverdicted novelty 5.0

    Line ratio diagnostics in NGC 1068 indicate AGN outflows are shock-accelerated, with outflowing gas dust-free and 19-110 times denser than disk gas.

  2. Revisiting the mass metallicity relation and the fundamental metallicity relation of dwarf galaxies at cosmic noon with NIRISS

    astro-ph.GA 2026-05 conditional novelty 5.0

    JWST observations confirm a constant-slope mass-metallicity relation for high-redshift dwarf galaxies down to 10^6.3 solar masses with no clear fundamental metallicity relation.

  3. Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068

    astro-ph.GA 2026-06 unverdicted novelty 4.0

    Line ratio diagnostics in NGC 1068 indicate that AGN outflows are accelerated by shocks that destroy dust and compress gas.