Isolated dwarf galaxies: From cuspy to flat dark matter density profiles and metalicity gradients

被引：0
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作者：
Pasetto, S. [1 ,2 ]
Grebel, E.K. [1 ]
Berczik, P. [1 ,3 ,4 ]
Spurzem, R. [1 ,3 ,5 ]
Dehnen, W. [6 ]
机构：
[1] Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität, Heidelberg, Germany
[2] Max-Planck-Institut für Astronomie, Heidelberg, Germany
[3] National Astronomical Observatories of China (NAOC), Chinese Academy of Sciences (CAS), Datun Lu 20A, Chaoyang District, Beijing 100012, China
[4] Main Astronomical Observatory (MAO), National Academy of Sciences of Ukraine (NASU), Akademika Zabolotnoho 27, 03680 Kyiv, Ukraine
[5] Kavli Institute of Astronomy and Astrophysics, Peking University, Beijing, China
[6] Department of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH, United Kingdom
来源：
Astronomy and Astrophysics | 2010年 / 514卷 / 05期
关键词：
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摘要：
Stars
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