de.mpg.escidoc.pubman.appbase.FacesBean
English
 
Help Guide Disclaimer Contact us Login
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

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

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons4923

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4590

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4584

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4768

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4582

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4586

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4766

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

Locator
There are no locators available
Fulltext (public)
There are no public fulltexts available
Supplementary Material (public)
There is no public supplementary material available
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: http://hdl.handle.net/11858/00-001M-0000-000F-49AB-F
Abstract
There is no abstract available