On the origin of star formation quenching in massive galaxies at z 3 in the cosmological simulations Illustris TNG

被引：0
|
作者：
Kurinchi-Vendhan, Shalini [1 ,2 ]
Farcy, Marion [3 ]
Hirschmann, Michaela [3 ,4 ]
Valentino, Francesco [5 ,6 ]
机构：
[1] California Institute of Technology (Caltech), 1200 E. California Boulevard, Pasadena,CA,91125, United States
[2] Max-Planck-Institut für Astronomie (MPIA), Königstuhl 17, Heidelberg, Baden-Württemberg,D-69117, Germany
[3] École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, Chemin Pegasi 51, Versoix,CH-1290, Switzerland
[4] Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Trieste, Via Tiepolo 11, Trieste,I-34131, Italy
[5] European Southern Observatory (ESO), Karl-Scwharzschild-Strasse 2, Garching bei München,D-85748, Germany
[6] Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Rådmandsgade 62-64, Copenhagen,DK-2200, Denmark
来源：
Monthly Notices of the Royal Astronomical Society | 2024年 / 534卷 / 04期
关键词：
D O I：
10.1093/mnras/stae2297
中图分类号：
学科分类号：
摘要：
Kinetic energy
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收藏
页码：3974 / 3988
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