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...
| Hlavní autoři: | , |
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| Médium: | Journal article |
| Vydáno: |
1996
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