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Intense star formation and feedback at high redshift: spatially resolved properties of the z = 2.6 submillimeter galaxy SMM J14011+0252

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Nesvadba,  N. P. H.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Seitz,  S.
Optical and Interpretative 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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Lutz,  D.
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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Bender,  R.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Nesvadba, N. P. H., Lehnert, M. D., Genzel, R., Eisenhauer, F., Baker, A. J., Seitz, S., et al. (2007). Intense star formation and feedback at high redshift: spatially resolved properties of the z = 2.6 submillimeter galaxy SMM J14011+0252. Astrophysical Journal, 658(2 Part 1), 725-737. doi:10.1086/511151.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-CE19-1
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