Morphological evolution of disc galaxies in chemodynamical simulations

被引:0
|
作者
Michel-Dansac, L. [1 ]
Wozniak, H. [1 ]
机构
[1] Univ Nacl Autonoma Mexico, Inst Astron, Ensenada, Baja California, Mexico
关键词
D O I
10.1051/eas:20070055
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Chemodynamical disc galaxy simulations coupled with stellar populations synthesis models allow to build multi-wavelength images from numerical simulations, and then to follow their morphological evolution in colour and not only on the mass distribution. Using such technique, we present the evolution of several photometric observables, of the Tully-Fisher relation, as well is the evolution of disc structural parameters.
引用
收藏
页码:39 / 44
页数:6
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