Mass Distribution in Rotating Thin-Disk Galaxies According to Newtonian Dynamics
An accurate computational method is presented for determining the mass distribution in a mature spiral galaxy from a given rotation curve by applying Newtonian dynamics for an axisymmetrically rotating thin disk of finite size with or without a central spherical bulge. The governing integral equatio...
Gardado en:
| Principais autores: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
MDPI AG
2014-04-01
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| Series: | Galaxies |
| Assuntos: | |
| Acceso en liña: | http://www.mdpi.com/2075-4434/2/2/199 |
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