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Enriched haloes at redshift z = 2 with no star formation: implications for accretion and wind scenarios

MPS-Authors
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Förster Schreiber,  N. M.
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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Lutz,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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

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Citation

Bouché, N., Murphy, M. T., Péroux, C., Contini, T., Martin, C. L., Förster Schreiber, N. M., et al. (2012). Enriched haloes at redshift z = 2 with no star formation: implications for accretion and wind scenarios. Monthly Notices of the Royal Astronomical Society, 419(1), 2-13. doi:10.1111/j.1365-2966.2011.19500.x.


Cite as: https://hdl.handle.net/11858/00-001M-0000-000F-49AB-F
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