期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 419, 期 3, 页码 2251-2263出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2011.19879.x
关键词
methods: data analysis; Galaxy: disc; solar neighbourhood; galaxies: evolution; galaxies: kinematics and dynamics
资金
- Science and Technology Facilities Council
- STFC [ST/G002479/1, ST/J00149X/1, PP/D001242/1] Funding Source: UKRI
- Science and Technology Facilities Council [PP/D001242/1, ST/J00149X/1, ST/G002479/1] Funding Source: researchfish
We consider what is the best way to extract science from large surveys of the Milky Way Galaxy. The diversity of data gathered in these surveys, together with our position within the Galaxy, implies that science must be extracted by fitting dynamical models to the data in the space of the observables. Models based on orbital tori promise to be superior for this task than traditional types of models, such as N-body models and Schwarzschild models. A formalism that allows such models to be fitted to data is developed and tested on pseudo-data of varying richness drawn from axisymmetric disc models.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据