机译:水动力模拟再现的星系性质
Department of Physics, Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA;
Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35,69118 Heidelberg, Germany,Zentrum fuer Astronomie der Universitaet Heidelberg, ARI, Moenchhofstrasse 12-14,69120 Heidelberg, Germany;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA;
Kavli Institute for Cosmology, and Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK;
Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35,69118 Heidelberg, Germany;
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA;
Institute for Advanced Study, 1 Einstein Drive, Princeton, New Jersey 08540, USA;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA;
机译:高红移星系在宇宙流体动力学模拟中的物理和光度学特性
机译:高倍率银河系在水力动力学模拟中的物理和光度特性
机译:高倍率星系在宇宙流动力学模拟中的物理和光度特性
机译:在流体动力学模拟中恢复数值可再现性
机译:使用再现内核插值方案和高性能计算平台可视化平滑粒子流体动力学模拟数据
机译:火星上的SIDM:低质量矮星系的水动力自相互作用暗物质模拟
机译:通过流体动力学模拟再现的星系属性