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The reversal of the star formation-density relation in the distant universe
Astronomy and Astrophysics · 2007 · Vol. 468(1) · pp. 33–48
D. Elbaz✉(Centre National de la Recherche Scientifique)E. Daddi(CEA Paris-Saclay)D. Le Borgne(CEA Paris-Saclay)Mark Dickinson(Kitt Peak National Observatory)D. M. Alexander(Durham University)Ranga‐Ram Chary(California Institute of Technology)Jean‐Luc Starck(Commissariat à l'Énergie Atomique et aux Énergies Alternatives)W. N. Brandt(Pennsylvania State University)Manfred G. Kitzbichler(Max Planck Institute for Astrophysics)Emily Macdonald(Kitt Peak National Observatory)M. Nonino(Trieste Astronomical Observatory)P. Popesso(European Southern Observatory)Daniel Stern(Jet Propulsion Laboratory)E. Vanzella(Trieste Astronomical Observatory)
Abstract
Aims.We study the relationship between the local environment of galaxies and their star formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at .
Galaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical ResearchScientific Research and DiscoveriesStar formationGalaxyStar (game theory)Relation (database)UniverseAstronomyAstrophysicsPhysicsGeographyComputer science
Funding
- California Institute of Technology
- Royal Society
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