Setting the scene for Gaia and LAMOST
Setting the scene for Gaia and LAMOST
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发表时间：
2014
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通讯作者：
S. Feltzing;Gang Zhao;N. Walton;P. Whitelock
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作者：
S. Feltzing;Gang Zhao;N. Walton;P. Whitelock
Feltzing Zhao Walton Whitelock为盖亚和LAMOST IAU研讨会设置场景2013年5月20日至24日中国丽江盖亚是一个雄心勃勃的卫星使命，绘制银河系的三维地图。通过测量10亿颗恒星的自行和自转，盖亚将改变我们研究银河系组成、形成和演化的方式。与此同时，中国的LAMOST测量设施将对北方大部分天空中的数百万个物体进行补充光谱测量。这卷，包括评论和贡献的会谈在IAU研讨会298，是一个最新的审查，我们知道银河系作为一个星系之前，盖亚发射。它涵盖了许多主题，从动态模拟的状态，光度和光谱调查，以及银河系中的星际物质和恒星大气的详细研究。专家评论将使所有从事银河系天文学以及星系形成和演化的人感兴趣。
Feltzing Zhao Walton Whitelock Setting the Scene for Gaia and LAMOST IAU Symposium No. 298 20-24 May 2013 Lijiang,China Gaia is an ambitious satellite mission to chart a three-dimensional map of the Milky Way. By measuring the proper motions and parallaxes for a billion stars, Gaia is set to transform the way we study the composition, formation and evolution of our galaxy. Concurrently the LAMOST survey facility in China will make a complementary spectral survey of millions of objects in much of the northern sky. This volume, comprising the reviews and contributed talks presented at IAU Symposium 298, is an up-to-date review of what we know about the Milky Way as a galaxy prior to the launch of Gaia. It covers many topics ranging from the status of dynamical simulations, photometric and spectroscopic surveys, as well as interstellar matter in the Milky Way and detailed studies of stellar atmospheres. The expert reviews will interest all those working on Milky Way astronomy as well as galaxy formation and evolution.