Milky Way Dark Matter Distribution or MOND Test from Vertical Stellar Kinematics with Gaia DR3
Vertical stellar kinematics+density can be used to trace the dark matter distribution (or the equivalent phantom mass in a Modified Newtonian Dynamics (MOND) scenario) through the Jeans equations. In this paper, we want to improve this type of analysis by making use of the recent data of the 6D info...
Saved in:
| Main Author: | Martín López-Corredoira |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad94f5 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Kinematic Signature of the Warp and Waves in the Milky Way Disk
by: Weixiang Sun, et al.
Published: (2025-01-01) -
The Structure, Populations, and Kinematics of the Milky Way Central and Inner Bulge with OGLE, APOGEE, and Gaia Data
by: Xiao Han, et al.
Published: (2025-01-01) -
The Age–Velocity Dispersion Relations of the Galactic Disk as Revealed by the LAMOST-Gaia Red Clump Stars
by: Weixiang Sun, et al.
Published: (2025-01-01) -
Cosmological Predictions for Minor Axis Stellar Density Profiles in the Inner Regions of Milky Way–mass Galaxies
by: Madeline Lucey, et al.
Published: (2025-01-01) -
GD-1 and the Milky Way Starless Dark Matter Subhalos
by: Raymond G. Carlberg
Published: (2025-01-01)