The Mass Distribution and Assembly of the Milky Way from the Properties of the Magellanic Clouds
We present a new measurement of the mass of the Milky Way (MW) based on observed properties of its largest satellite galaxies, the Magellanic Clouds (MCs), and an assumed prior of a {\Lambda}CDM universe. The large, high-resolution Bolshoi cosmological simulation of this universe provides a means to...
| المؤلفون الرئيسيون: | , , , , |
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| التنسيق: | Journal article |
| منشور في: |
2010
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