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...
मुख्य लेखक: | Yoshiaki Sofue |
---|---|
स्वरूप: | लेख |
भाषा: | English |
प्रकाशित: |
MDPI AG
2020-04-01
|
श्रृंखला: | Galaxies |
विषय: | |
ऑनलाइन पहुंच: | https://www.mdpi.com/2075-4434/8/2/37 |
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