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Molecular and ionized gas phases of an AGN-driven outflow in a typical massive galaxy at z ≈ 2

MPS-Authors
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Herrera-Camus,  R.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons4582

Tacconi,  L.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons4590

Genzel,  R.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons4923

Foerster Schreiber,  N.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons4584

Lutz,  D.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons187981

Belli,  S.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons128736

Übler,  H.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons206401

Shimizu,  T.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons208361

Davies,  R.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons4650

Sturm,  E.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons16252

Naab,  T.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Citation

Herrera-Camus, R., Tacconi, L., Genzel, R., Foerster Schreiber, N., Lutz, D., Bolatto, A., et al. (2019). Molecular and ionized gas phases of an AGN-driven outflow in a typical massive galaxy at z ≈ 2. The Astrophysical Journal, 871(1): 37, pp. 1-18. doi:10.3847/1538-4357/aaf6a7.


Cite as: https://hdl.handle.net/21.11116/0000-0003-5CC0-D
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