Mass models of the Milky Way
A parameterized model of the mass distribution within the Milky Way is fitted to the available observational constraints. The most important single parameter is the ratio of the scale length R_d* of the stellar disk to R0. The disk and bulge dominate v_c(R) at R<r0 0.3.="" <<=&quo...
| Principais autores: | , |
|---|---|
| Formato: | Journal article |
| Publicado em: |
1996
|
Search Result 1
