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...
מחבר ראשי: | Yoshiaki Sofue |
---|---|
פורמט: | Article |
שפה: | English |
יצא לאור: |
MDPI AG
2020-04-01
|
סדרה: | Galaxies |
נושאים: | |
גישה מקוונת: | https://www.mdpi.com/2075-4434/8/2/37 |
פריטים דומים
-
The Circular Velocity Curve of the Milky Way from 5–25 kpc Using Luminous Red Giant Branch Stars
מאת: Yuan Zhou, et al.
יצא לאור: (2023-01-01) -
The Milky way & other stellar systems [slaid]
יצא לאור: (197-) -
Generalized Rotation Curves of the Milky Way from the GAIA DR3 Data Set: Constraints on Mass Models
מאת: Francesco Sylos Labini
יצא לאור: (2024-01-01) -
Two-point Correlation Function Studies for the Milky Way: Discovery of Spatial Clustering from Disk Excitations and Substructure
מאת: Austin Hinkel, et al.
יצא לאור: (2023-01-01) -
Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set
מאת: Francesco Sylos Labini, et al.
יצא לאור: (2023-01-01)