A POSSIBLE LOCAL DIAGNOSTIC FOR THE MILKY WAY DARK MATTER HALO TRIAXIALITY
In this study we propose to constrain through the local stellar kinematics, the overall shape of the Milky Way dark matter halo. We base on the principle that the shape of the halo implies the existence of families of periodic orbits that support the triaxial shape. These groups would appear as kine...
Αποθηκεύτηκε σε:
| Εκδόθηκε σε: | Revista Mexicana de Astronomía y Astrofísica |
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| Κύριοι συγγραφείς: | , , |
| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
Universidad Nacional Autónoma de México
2011
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| Θέματα: | |
| Διαθέσιμο Online: | https://www.redalyc.org/articulo.oa?id=57121297037 |
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