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...

Descrición completa

Detalles Bibliográficos
Autor Principal: Yoshiaki Sofue
Formato: Artigo
Idioma:English
Publicado: MDPI AG 2020-04-01
Series:Galaxies
Subjects:
Acceso en liña:https://www.mdpi.com/2075-4434/8/2/37

Títulos similares