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...
Päätekijä: | |
---|---|
Aineistotyyppi: | Artikkeli |
Kieli: | English |
Julkaistu: |
MDPI AG
2020-04-01
|
Sarja: | Galaxies |
Aiheet: | |
Linkit: | https://www.mdpi.com/2075-4434/8/2/37 |