Rotation Curve of the Milky Way and the Dark Matter Density

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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Dades bibliogràfiques
Autor principal:	Yoshiaki Sofue
Format:	Article
Idioma:	English
Publicat:	MDPI AG 2020-04-01
Col·lecció:	Galaxies
Matèries:	galaxies DM—galaxies individual (Milky Way)—galaxies rotation curve
Accés en línia:	https://www.mdpi.com/2075-4434/8/2/37

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