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...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Pontificia Universidad Javeriana
2018-07-01
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Series: | Universitas Scientiarum |
Subjects: | |
Online Access: | https://revistas.javeriana.edu.co/index.php/scientarium/article/view/20059 |