Mass of Spiral Galaxies by Means of a Maximum Disc Model
Maximum disc mass models for a set of spiral galaxies from the Ursa Major Cluster are presented. We construct the models using the Hunther method and the particular solutions are chosen in such away that the circular velocities are adjusted very accurately to the observed rotation curves of some spe...
Saved in:
| Main Authors: | Framsol López-Suspes, Guillermo A González |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Pontificia Universidad Javeriana
2018-07-01
|
| Series: | Universitas Scientiarum |
| Subjects: | |
| Online Access: | https://revistas.javeriana.edu.co/index.php/scientarium/article/view/20059 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Rotating Bulge and Halo in the Milky Way: Evidence of Angular Momentum Transferred from the Decelerating Bar
by: Zhuohan Li, et al.
Published: (2025-01-01) -
The Expanding 3 kpc Arms Are Neither Expanding nor Spiral Arms but X1 Orbits Driven by the Galactic Bar
by: Jayender Kumar, et al.
Published: (2025-01-01) -
StarFlow: Leveraging Normalizing Flows for Stellar Age Estimation in SDSS-V DR19
by: Alexander Stone-Martinez, et al.
Published: (2025-01-01) -
On the Formation of S stars from a Recent Massive Black Hole Merger in the Galactic Center
by: Tatsuya Akiba, et al.
Published: (2025-01-01) -
Extreme-mass-ratio Inspirals in the Strong Segregation Regime—to Inspiral or to Get Ejected?
by: Karamveer Kaur, et al.
Published: (2024-01-01)