The reversal of the star formation-density relation in the distant universe
D. ElbazAIM-Unité Mixte de Recherche CEA-CNRS (#7158)-Université Paris VII, FranceE. DaddiAIM-Unité Mixte de Recherche CEA-CNRS (#7158)-Université Paris VII, FranceD. Le BorgneAIM-Unité Mixte de Recherche CEA-CNRS (#7158)-Université Paris VII, FranceMark DickinsonNational Optical Astronomy Observatory, 950 North Cherry Street, Tucson, AZ 85719, USAD. M. AlexanderDepartment of Physics, Durham University, South Road, Durham, DH13LE, UKRanga‐Ram CharySpitzer Science Center, California Institute of Technology, Pasadena, CA 91125, USAJean‐Luc StarckCEA-Saclay, DSM/DAPNIA/Service d'Astrophysique, 91191 Gif-sur-Yvette Cedex, France e-mail: [email protected]W. N. BrandtDepartment of Astronomy and Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, Pennsylvania, PA 16802, USAManfred G. KitzbichlerMax-Planck Institute of Astrophysics, Karl-Schwarzschild Str. 1, PO Box 1317, 85748 Garching, GermanyEmily MacdonaldNational Optical Astronomy Observatory, 950 North Cherry Street, Tucson, AZ 85719, USAM. NoninoINAF – Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 40131 Trieste, ItalyP. PopessoEuropean Southern Observatory, Karl Schwarzschild Strasse 2, Garching bei Muenchen 85748, GermanyDaniel SternJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USAE. VanzellaINAF – Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 40131 Trieste, Italy
2007en
ABI
Аннотация
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 .
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Цитирований: 2Использованных источников: 0