English
 
User Manual Privacy Policy Disclaimer Contact us
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

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

MPS-Authors
/persons/resource/persons23694

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

/persons/resource/persons23427

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

/persons/resource/persons4590

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

/persons/resource/persons4766

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

/persons/resource/persons18405

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

/persons/resource/persons4586

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

/persons/resource/persons4584

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

/persons/resource/persons4582

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

/persons/resource/persons4759

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

External Ressource
No external resources are shared
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
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: http://hdl.handle.net/11858/00-001M-0000-0011-CE19-1
Abstract
There is no abstract available