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...
| Egile nagusia: | |
|---|---|
| Formatua: | Artikulua |
| Hizkuntza: | English |
| Argitaratua: |
MDPI AG
2020-04-01
|
| Saila: | Galaxies |
| Gaiak: | |
| Sarrera elektronikoa: | https://www.mdpi.com/2075-4434/8/2/37 |