Rotation Curve of the Milky Way and the Dark Matter Density
We review the current status of the study of rotation curve (RC) of the Milky Way, and present a unified RC from the Galactic Center to the galacto-centric distance of about 100 kpc. The RC is used to directly calculate the distribution of the surface mass density (SMD). We then propose a method to...
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| Formato: | Artigo |
| Idioma: | English |
| Publicado em: |
MDPI AG
2020-04-01
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| coleção: | Galaxies |
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| Acesso em linha: | https://www.mdpi.com/2075-4434/8/2/37 |