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Properties of galaxies reproduced by a hydrodynamic simulation.
Vogelsberger, M; Genel, S; Springel, V; Torrey, P; Sijacki, D; Xu, D; Snyder, G; Bird, S; Nelson, D; Hernquist, L.
Afiliação
  • Vogelsberger M; Department of Physics, Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.
  • Genel S; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA.
  • Springel V; 1] Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany [2] Zentrum für Astronomie der Universität Heidelberg, ARI, Mönchhofstrasse 12-14, 69120 Heidelberg, Germany.
  • Torrey P; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA.
  • Sijacki D; Kavli Institute for Cosmology, and Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK.
  • Xu D; Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany.
  • Snyder G; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA.
  • Bird S; Institute for Advanced Study, 1 Einstein Drive, Princeton, New Jersey 08540, USA.
  • Nelson D; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA.
  • Hernquist L; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA.
Nature ; 509(7499): 177-82, 2014 May 08.
Article em En | MEDLINE | ID: mdl-24805343
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2014 Tipo de documento: Article
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2014 Tipo de documento: Article