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Rotating starburst cores in massive galaxies at z = 2.5

MPS-Authors
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Tadaki,  Ken-ichi
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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

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Förster Schreiber,  Natascha M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Herrera-Camus,  Rodrigo
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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

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

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

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

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

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Citation

Tadaki, K.-i., Kodama, T., Nelson, E. J., Belli, S., Förster Schreiber, N. M., Genzel, R., et al. (2017). Rotating starburst cores in massive galaxies at z = 2.5. The Astrophysical Journal Letters, 841(2): L25. doi:10.3847/2041-8213/aa7338.


Cite as: http://hdl.handle.net/11858/00-001M-0000-002D-BBC7-5
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