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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Hlavní autor: Yoshiaki Sofue
Médium: Článek
Jazyk:English
Vydáno: MDPI AG 2020-04-01
Edice:Galaxies
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On-line přístup:https://www.mdpi.com/2075-4434/8/2/37

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