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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.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Tacconi,  L.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Genzel,  R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Foerster Schreiber,  N.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lutz,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Belli,  S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Übler,  H.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Shimizu,  T.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Davies,  R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Sturm,  E.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Burkert,  A.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, 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. doi:10.3847/1538-4357/aaf6a7.


Cite as: http://hdl.handle.net/21.11116/0000-0003-0F4E-7
Abstract
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